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| | Shropshire Astronomical Society - Deep Sky Images page |
 | | This image was taken by Kev Wildgoose using a 12" Newtonian and MX916 CCD camera. | | | As imaged by Kev Wildgoose using his 16" Newtonian and a Starlight MX916 CCD camera on 26 April 2001. | | | On the left is a monochrome image taken with an 8" F4.5 Newtonian and a TC255 based CCD by Grant Privett. |
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http://www.astro.cf.ac.uk/sas/galaxy.htm
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| | Galaxy Hopping Though Leo the Lion |
| | The hop is an easy one, moving south about 2-3 degrees to 5th magnitude 73 Leonis and one degree east to the galaxies. | | | This may be 1 or 2 fields of view away from 52 Leonis depending on your telescope and eyepiece combination. | | | A magnitude 6.9 star is immediately to the north of M65 and M66. |
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http://www.fvastro.org/beginners/galaxy_hopping_leo.htm
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| | * M95 - (Astronomy): Definition |
| | The large dynamic range of the CCD can capture all of this but the human eye or film will be dominated entirely by its bright center | | | M95 is a member of the, which also contains M96, and a number of fainter galaxies. | | | This image was created by from B,V,R images obtained on the 4. |
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http://en.mimi.hu/astronomy/m95.html
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| | Spiral (and other Disk) Galaxies |
| | the disk around the center of M87, which is often regarded as the accretion disk around the supermassive object in that galaxy's nucleus, may be a smaller manifestation of the same disk phenomenon. | | | our illustration of the Hubble Scheme with Messier galaxies). | | | These structures have been a mystery for a long time, it was thought that there may be physically different classes of disks (e.g., "normal" and "barred" disks), but now it seems as if they are all the consequences of gravitational interactions with neighboring galaxies. |
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http://www.seds.org/messier/spir.html
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| | Spiral Galaxy M95 - Digital Picture Printing & Frames |
| | Unfortunately, our Frameshop cannot be used unless you have a Javascript-enabled browser. | | | Spiral Galaxy M95 - Digital Picture Printing and Frames | | | Or, you can return to the main page and continue shopping. |
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http://www.digital-picture-printing-frames.com/frame_image.asp?product_ID=4105
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| | Spiral Galaxy M95 (NGC 3351) |
| | The bright spiral galaxy Messier 95 (NGC 3351) in Leo, shown from a red-light CCD exposure with an RCA CCD at the 1.1-meter Hall telescope of Lowell Observatory. | | | The field is 3.6 by 6.0 arcminutes, which doesn't cover the whole galaxy (the bigger TI CCDs had gone to Australia at the time, to support observations of the Shoemaker-Levy 9 impact). | | | This display uses a logarithmic intensity transformation to preserve information across a wide dynamic range. |
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http://www.astr.ua.edu/gifimages/m95r.html
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| | M95-M96 |
| | Exposure: LRGB: L 10 x 4 minutes, binned 1x1: R 4 x 6 minutes: G 3 x 6 minutes: B 5 x 6 minutes: RGB binned 2x2 | | | Moderately large telescopes are required to see the spiral structures. | | | Located 38 million light-years from the solar system, they are visible in binculars and small telescopes. |
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http://webpages.charter.net/alsonwongweb/m95-m96.htm
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| | Messier Object 95 |
| | A preliminary result has been obtained and published in 1996-97 by the HST H0 Key Project Team (paper VII, 1997). | | | M95 is a barred spiral of type SBb, or SB(r)ab according to de Vaucouleurs' classification, with nearly circular arms. | | | M95 is a member of the Leo I or M96 group, which also contains M96, M105 and a number of fainter galaxies. |
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http://www.seds.org/messier/m/m095.html
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| | Spiral Galaxy M95 - Wikipedia, the free encyclopedia |
| | M96 group, which is sometimes known as the Leo I group. | | | This page was last modified 06:41, 7 Jan 2005. | | | The Spiral Galaxy M95 (also known as Messier Object 95, Messier 95, M95, or NGC 3351) is a spiral galaxy (type SBb) in the |
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http://en.wikipedia.org/wiki/Spiral_Galaxy_M95
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| | NGC 3351, Messier 95 |
| | While the 'bar' is the dominant feature in a picture taken from afar, it is easy to imagine that this structure could be very difficult to detect from inside the galaxy, especially if seen from a position at right angles to it. | | | Though the exact form of our own galaxy, the Milky Way, is not known, there is increasing evidence that it is a barred spiral, perhaps like M95. | | | Despite the distance, several of these galaxies appear in Messier's catalogue, about one third of which consists of galaxies. |
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http://www.aao.gov.au/images/captions/aat097.html
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| | M-95, barred Spiral Galaxy |
| | This cluster includes other bright members, like spiral galaxies M-65 and M-66, plus numerous smaller systems. | | | Note that the spiral arms do continue on into very faint extensions. | | | There are three major complexes of H-II regions, whose high content of O stars gives a young age to the burst. |
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http://www.kopernik.org/images/archive/m95.htm
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| | M95 |
| | This galaxy, which is part of the Leo | | | cluster of galaxies, is about 38,000,000 light years away. |
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http://astroimage.homestead.com/M95.html
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| | Talk:M96 group of galaxies - Wikipedia, the free encyclopedia |
| | This page was last modified 21:22, 8 Sep 2004. | | | Elliptical Galaxy M105, and a number of fainter galaxies. | | | Leo I (or the M96 group) is a physical group of galaxies in the constellation Leo consisting of Spiral Galaxy M95, Spiral Galaxy M96, |
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http://en.wikipedia.org/wiki/Talk:M96_group_of_galaxies
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| | Leo (abbr. Leo, gen. Leonis) |
| | An edge-on type Sb spiral that forms a conspicuous triple with M66 and NGC 3628. | | | A face-on type SBb barred spiral that forms a pair with M96 (see Leo I). | | | A physical partner of M65 and another edge-on Sb spiral. |
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http://www.daviddarling.info/encyclopedia/L/Leo_constellation.html
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| | M95 Barred Spiral Galaxy |
| | : M95 is a barred spiral galaxy located in the Constellation Leo at an approximate distance of 26.5 million light-years. | | | This galaxy exhits a strong central bar with circular spiral arms. |
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http://www.ironmountainobservatory.com/photos/singles/M95galaxy.html
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