mirror of https://github.com/XEphem/XEphem.git
908 lines
17 KiB
Plaintext
908 lines
17 KiB
Plaintext
<gallery>
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<image>
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<name>
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NGC 2207
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</name>
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<file>
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1999-41-a-web_print.jpg
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</file>
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<description>
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In the direction of the
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constellation Canis Major, two spiral galaxies pass by each other like
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majestic ships in the night. The near-collision has been caught in images
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taken by NASA's Hubble Space Telescope and its Wide Field Planetary Camera 2.
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The larger and more massive galaxy is cataloged as NGC 2207 (on the left in the
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Hubble Heritage image), and the smaller one on the right is IC 2163. Strong
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tidal forces from NGC 2207 have distorted the shape of IC 2163, flinging
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out stars and gas into long streamers stretching out a hundred thousand
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light-years toward the right-hand edge of the image.
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Computer simulations, carried out by a team led by Bruce and Debra Elmegreen,
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demonstrate the leisurely timescale over which galactic collisions occur. In
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addition to the Hubble images, measurements made with the National Science
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Foundation's Very Large Array Radio Telescope in New Mexico reveal the
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motions of the galaxies and aid the reconstruction of the collision.
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The calculations indicate that IC 2163 is swinging past NGC 2207 in a
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counterclockwise direction, having made its closest approach 40 million
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years ago. However, IC 2163 does not have sufficient energy to escape from
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the gravitational pull of NGC 2207, and is destined to be pulled back and
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swing past the larger galaxy again in the future.
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The high resolution of the Hubble telescope image reveals dust lanes in
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the spiral arms of NGC 2207, clearly silhouetted against IC 2163, which is
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in the background. Hubble also reveals a series of parallel dust filaments
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extending like fine brush strokes along the tidally stretched material on the
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right-hand side. The large concentrations of gas and dust in both galaxies
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may well erupt into regions of active star formation in the near future.
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Trapped in their mutual orbit around each other, these two galaxies will
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continue to distort and disrupt each other. Eventually, billions of years
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from now, they will merge into a single, more massive galaxy. It is believed
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that many present-day galaxies, including the Milky Way, were assembled from
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a similar process of coalescence of smaller galaxies occurring over billions
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of years.
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This image was created from 3 separate pointings of Hubble. The Wide Field
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Planetary Camera 2 data sets were obtained by Debra Meloy Elmegreen (Vassar
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College), Bruce G. Elmegreen (IBM Research Division), Michele Kaufman (Ohio
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State U.), Elias Brinks (Universidad de Guanajuato, Mexico), Curt Struck (Iowa
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State University), Magnus Thomasson (Onsala Space Obs., Sweden), Maria Sundin
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(Goteborg University, Sweden), and Mario Klaric (Columbia, South Carolina).
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Credit: NASA and Hubble Heritage Team (STScI)
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</description>
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</image>
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<image>
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<name>
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Virgo cluster
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</name>
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<file>
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pui-17-virgo-anno1000.jpg
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</file>
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<description>
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Virgo Galaxy Cluster
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Puimichel, 14-15 May, 2002
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135/2.8 lens at f/4, 15 min, Kodak Supra 400
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This photo covers most of the Virgo Cluster, the most nearby massive galaxy
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cluster. Dozens of small galaxies are visible in this photo. All galaxies
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brighter than magnitude 12 has been labelled
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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NGC 6819
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</name>
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<file>
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ngc6819-25aug01-lrgb.jpg
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</file>
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<description>
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NGC 6819 in Cygnus
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Magnitude 7,3 - Size 5'
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25 Aug 2001 - C8-DX at f/6.3 - MX516 - L:R:G:B = 2:1,5:1:1 min
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A nice compact open cluster in Cygnus
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M29
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</name>
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<file>
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m29-2002sep05.jpg
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</file>
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<description>
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M29 in Cygnus
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Magnitude 6,6 - Size 7,0'
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05 Sep 2002 - FFC 3.5/500 - MX516 - 6 min in high-res mode
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One of the less impressive Messier objects. Loose group of distant but very hot stars.
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M103
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</name>
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<file>
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m103-2002sep13-lrgb.jpg
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</file>
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<description>
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M103 in Cassiopeia
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Magnitude 7,4 - Size 6,0' - 40 stars
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13 Sep 2002 - FFC 3.5/500 - LRGB = 6:4:3:4 min - high res mode
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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NGC 457
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</name>
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<file>
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ngc457-2002sep13-lrgb.jpg
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</file>
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<description>
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NGC 457 (Owl Cluster) in Cassiopeia
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Magnitude 6,4 - Size 13' - 80 stars
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13 Sep 2002 - FFC 3.5/500 - LRGB = 6:4:2:7 min - high res mode
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This cluster is sometimes nicknamed the "ET Cluster" and it really looks like
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an alien with those two "eyes". The brightest star is phi Cass. and is not a
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member of the cluster.
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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NGC 869
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</name>
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<file>
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ngc869-2002oct06-lrgb.jpg
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</file>
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<description>
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NGC 869/884, The Double Cluster in Perseus
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Magnitude 5,3/6,1 - Size 30'/30'
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06 Oct 2002 - FFC 3.5/500 - MX516 - Mosaic of 4 images - Each image LRGB = 7:2:2:2 min in high res mode
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The Double Cluster is a naked eye object under a moderately dark sky. It is
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therefore quite surprising that Messier missed it in his famous catalogue.'-
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M35
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</name>
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<file>
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m35-11dec01-grgb.jpg
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</file>
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<description>
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M35 in Gemini
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Magnitude 5,1 - Size 28'
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11 Dec 2001 - ST80 (42 mm aperture) - MX516 - (L)RGB = 210:270:150 sec (30 sec
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exposures) - L = G
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Large open cluster that is a good binocular target. I missed the little
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distant cluster NGC2158 that is located just off the lower right corner. The
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ST80 was stopped down to reduce the colour error. Further the green image was
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used as the luminance channel since it has the best focus. Bright blue stars
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do get a halo probably due to a violet or UV leak in the green filter
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M76
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</name>
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<file>
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m76-07dec01-lrgb-nr.jpg
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</file>
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<description>
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M76 (Little Dumbbell) in Perseus
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Magnitude 11,0 - Size 2,7' x 1,8'.
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L: 14 Nov 2001 - C8 at f/6.3 - MX516 - 510 sec
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RGB: 07 Dec 2001 - R:G:B = 120:120:120 sec - LRGB
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This is the faintest of all Messier objects but its rather high surface
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brightness makes it more easy to observe than should be expected from its
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magnitude. My first try (14 Nov) using the ST80 as guide scope (see equipment)
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M97
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</name>
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<file>
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m97-03apr02-lrgb.jpg
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</file>
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<description>
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M97 (Owl Nebula) in Ursa Major
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Magnitude 11,0 - Size 3,4' x 3,3'
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03 Apr 2002 - C8-DX at f/6.3 - MX516 - L:R:G:B = 13.5:6:7:6.5 min
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Low surface brightness planetary that is difficult to observe from my
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location. New colour version.
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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IC 5146
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</name>
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<file>
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ic5146-2002sep12-hall.jpg
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</file>
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<description>
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IC 5146 (Cocoon Nebula) in Cygnus
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12 Sep 2002 - FFC 3.5/500 - MX516 - lum: 14 min, h-alpha: 26 min - pseudo-rgb
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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NGC 6888
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</name>
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<file>
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ngc6888-27jul02-ha.jpg
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</file>
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<description>
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NGC 6888, The Crescent Nebula in Cygnus
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Magnitude 10,0 - Size 20' x 10'
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27 Jul 2002 - 135/2.8 lens at f/2.8 - MX516 - h-alpha filter - 16 min
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The Crescent nebula is a rare kind of nebulosity that has been created by a
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Wolf-Rayet star located at the center of the nebula. W-R stars represent the
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final stage in the evolution of supermassive stars before they explode as type
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Ib/Ic supernovae. Before and during the W-R phase the star blows off a large
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part of its mass in strong stellar winds forming an emission nebula around the
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hot star. Only 227 W-R stars are known in our galaxy
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M92
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</name>
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<file>
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m92-01jun02.jpg
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</file>
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<description>
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M92 (NGC 6341) in Hercules
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Magnitude 6,4 - Size 12,2'
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01 Jun 2002 - C8-DX at f/6.3 - MX516 - 10 min
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The "other" globular in Hercules. This beauty is somewhat overshadowed by its much more famous neighbour M13
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M3
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</name>
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<file>
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m3-2003may07-ddp.jpg
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</file>
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<description>
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M3 (NGC 5272) in Canes Venatici
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Magnitude 6,2 - Diameter 18,6'
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07 May 2003 - C8 at f/6.3 - MX516 - 26 min in high-res mode - DDP
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Together with M53 and M5 the prelude to the summer display of globular clusters.
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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M82
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</name>
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<file>
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m82-03apr02-rgb.jpg
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</file>
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<description>
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03 Apr 2002 C8 f/6.3 - R:G:B = 6.5:7:7 min (30 sec exposures) - denoised
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Credit: <20> Ole Nielsen 1999-2003 http://home.planet.nl/~onielsen
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</description>
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</image>
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<image>
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<name>
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Arp 295
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</name>
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<file>
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arp295_kelly_c1.jpg
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</file>
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<description>
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A spectacular bridge of stars and gas stretches for nearly 250,000 light-years
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and joins this famous peculiar pair of galaxies cataloged as Arp 295. The
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cosmic bridge between the galaxies and the long tail extending below and right
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of picture center are strong evidence that these two immense star systems have
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passed close to each other in the past, allowing violent tides induced by
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mutual gravity to create the eye-catching plumes of stellar material. While
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such interactions are drawn out over billions of years, repeated close
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passages should ultimately result in the merger of this pair of galaxies into
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a larger single galaxy of stars. Although this scenario does look peculiar,
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galactic mergers are thought to be common, with Arp 295 representing an early
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stage of this inevitable process. The Arp 295 pair are the largest of a loose
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grouping of galaxies about 270 million light-years distant toward the
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constellation Aquarius.
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Credit: This deep color image of the region was recorded in September using
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the USNO 1 meter telescope near Flagstaff, Arizona.
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</description>
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</image>
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<image>
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<name>
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NGC 7129
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</name>
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<name>
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NGC 7142
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</name>
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<file>
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N7129-2.jpg
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</file>
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<description>
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NGC 7129
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Object type: open cluster + reflection nebula
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Size: 8'
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Magnitude: 11.5 mag
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Constellation: Cep
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Distance: 3.300 Ly
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NGC 7142
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Object type: open cluster (II2r)
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Size: 4'
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Magnitude: 9.3 mag
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Constellation: Cep
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Distance: 3.300 Ly
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Credit: Bernhard Hubl, http://hubble.heim.at.
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</description>
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</image>
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<image>
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<name>
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NGC 7023
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</name>
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<name>
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Iris Nebula
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</name>
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<file>
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N7023-2.jpg
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</file>
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<description>
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NGC 7023
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Object type: open cluster + reflection nebula
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Size: 18'
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Magnitude: 7 mag
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Constellation: Cep
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Distance: 900 Ly
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Credit: Bernhard Hubl, http://hubble.heim.at.
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</description>
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</image>
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<image>
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<name>
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Sh2-115
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</name>
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<name>
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Abell 71
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</name>
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<file>
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S115-1.jpg
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</file>
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<description>
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Sh2-115
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Object type: emission nebula (HII)
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Size: 50'
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Constellation: Cyg
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Abell 71
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Object type: planetary nebula
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Size: 2.6'
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Magnitude: 15.2 mag
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Constellation: Cyg
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Credit: Bernhard Hubl, http://hubble.heim.at.
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</description>
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</image>
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<image>
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<name>
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NGC 6946
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</name>
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<name>
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NGC 6939
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</name>
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<file>
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N6946-1.jpg
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</file>
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<description>
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NGC 6946
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Object type: galaxy (SBc)
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Size: 11.2' x 9.8' ( >16' in negative image)
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Magnitude: 9.7 mag
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Constellation: Cep / Cyg
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Distance: 18 MLy
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NGC 6939
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Object type: open cluster (I1m)
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Size: 8'
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Magnitude: 7.8 mag
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Constellation: Cep
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Distance: 6,000 Ly
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Credit: Bernhard Hubl, http://hubble.heim.at.
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</description>
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</image>
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<image>
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<name>
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NGC 6791
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</name>
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<file>
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N6791-1.jpg
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</file>
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<description>
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NGC 6791
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Object type: open cluster (II3r)
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Size: 16'
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Magnitude: 9.5 / brightest star 13 mag
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Constellation: Lyr
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Distance: 17,000 Ly
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Credit: Bernhard Hubl, http://hubble.heim.at.
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</description>
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</image>
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<image>
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<name>
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NGC 6820
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</name>
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<name>
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Elephant's trunk
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</name>
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<file>
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N6820-2.jpg
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</file>
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<description>
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NGC 6820
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Object type: emission nebula
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Size: 40'
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Magnitude: 15,0
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Constellation: Vul
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Credit: Bernhard Hubl, http://hubble.heim.at.
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</description>
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</image>
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<image>
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<name>
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NGC 6040
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</name>
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<name>
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NGC 6041
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</name>
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<name>
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NGC 6043
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</name>
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<name>
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NGC 6045
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</name>
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<name>
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NGC 6050
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</name>
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<name>
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IC1178
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</name>
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<name>
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IC1181
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</name>
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<name>
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Hercules Galaxy Cluster
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</name>
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<name>
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Abell2151
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</name>
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<file>
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abell2151-1.jpg
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</file>
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<description>
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Hercules Galaxy Cluster
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Object type: galaxy cluster (87 members)
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Size: 128'
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Magnitude: brightest member: 14.4 mag
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Constellation: Her
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Distance: 500 MLy
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Credit: Bernhard Hubl, http://hubble.heim.at.
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</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
NGC 6633
|
||
</name>
|
||
<file>
|
||
N6633-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
NGC 6633
|
||
|
||
Object type: open cluster (III 2 m)
|
||
|
||
Size: 27'
|
||
|
||
Magnitude: 4.6 mag
|
||
|
||
Constellation: Oph
|
||
|
||
Distance: 1,100 Ly
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
M53
|
||
</name>
|
||
<name>
|
||
NGC 5053
|
||
</name>
|
||
<file>
|
||
M053-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
M53
|
||
|
||
Object type: globular cluster (V)
|
||
|
||
Size: 14.4'
|
||
|
||
Magnitude: 7.6 mag
|
||
|
||
Constellation: Com
|
||
|
||
Distance: 65,000 Ly
|
||
|
||
NGC 5053
|
||
|
||
Object type: globular cluster (XI)
|
||
|
||
Size: 8.9'
|
||
|
||
Magnitude: 9.5 mag
|
||
|
||
Constellation: Com
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
M 13
|
||
</name>
|
||
<name>
|
||
Hercules Cluster
|
||
</name>
|
||
<file>
|
||
M013-2.jpg
|
||
</file>
|
||
<description>
|
||
|
||
Object type: globular cluster (V)
|
||
|
||
Size: 16.6'
|
||
|
||
Magnitude: 5.9 mag
|
||
|
||
Constellation: Her
|
||
|
||
Distance: 22000 Ly
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
Hickson 68
|
||
</name>
|
||
<name>
|
||
NGC 5371
|
||
</name>
|
||
<file>
|
||
hickson68-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
Object type: galaxy group
|
||
|
||
Size: 10'
|
||
|
||
Magnitude: brightest member: 12,1 mag
|
||
|
||
Constellation: CVn
|
||
|
||
Distance: 100 MLy
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
Coma Galaxy Cluster
|
||
</name>
|
||
<name>
|
||
Abell 1656
|
||
</name>
|
||
<name>
|
||
NGC 4884
|
||
</name>
|
||
<name>
|
||
NGC 4874
|
||
</name>
|
||
<file>
|
||
abell1656-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
Coma Galaxy Cluster
|
||
|
||
Object type: galaxy cluster
|
||
|
||
Size: 180'
|
||
|
||
Magnitude: brightest member: 12.5 mag
|
||
|
||
Constellation: Com
|
||
|
||
Distance: 300 MLy
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
NGC 2174
|
||
</name>
|
||
<name>
|
||
NGC 2175
|
||
</name>
|
||
<file>
|
||
N2174-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
NGC 2174
|
||
|
||
Object type:emission nebula
|
||
|
||
Size: 40'
|
||
|
||
Constellation: Ori
|
||
|
||
open cluster NGC 2175 inside nebula
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
IC 1848
|
||
</name>
|
||
<file>
|
||
I1848-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
IC 1848
|
||
|
||
Object type: open cluster + emission nebula
|
||
|
||
Size: 60'
|
||
|
||
Magnitude: 6,5
|
||
|
||
Constellation: Cas
|
||
|
||
Distance: 2200 Ly
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
IC 2118
|
||
</name>
|
||
<name>
|
||
Witch Head Nebula
|
||
</name>
|
||
<file>
|
||
I2118-2.jpg
|
||
</file>
|
||
<description>
|
||
|
||
IC 2118
|
||
|
||
Object type: reflection nebula
|
||
|
||
Size: 180'
|
||
|
||
Constellation: Eri
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
IC 59
|
||
</name>
|
||
<name>
|
||
IC 63
|
||
</name>
|
||
<name>
|
||
Gamma Cas Nebulae
|
||
</name>
|
||
<file>
|
||
I0059-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
Gamma Cas Nebulae
|
||
|
||
Object type: reflection + emission nebula
|
||
|
||
Size: 10'
|
||
|
||
Constellation: Cas
|
||
|
||
Distance: 360 Ly
|
||
|
||
dark nebulae NW of Gamma Cas
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
IC 1613
|
||
</name>
|
||
<file>
|
||
I1613-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
IC 1613
|
||
|
||
Object type: galaxy (Irr)
|
||
|
||
Size: 16.6' x 14.9'
|
||
|
||
Magnitude: 9,9
|
||
|
||
Constellation: Cet
|
||
|
||
Distance: 5.5 MLy
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
|
||
<image>
|
||
<name>
|
||
M 34
|
||
</name>
|
||
<file>
|
||
M034-1.jpg
|
||
</file>
|
||
<description>
|
||
|
||
M 34
|
||
|
||
Object type: open cluster (II3m)
|
||
|
||
Size: 35'
|
||
|
||
Magnitude: 5,2
|
||
|
||
Constellation: Per
|
||
|
||
Distance: 1400 Ly
|
||
|
||
Credit: Bernhard Hubl, http://hubble.heim.at.
|
||
</description>
|
||
</image>
|
||
</gallery>
|