M81 Group
Template:Short description Template:Galaxy cluster
The M81 Group is a galaxy group in the constellations Ursa Major and Camelopardalis that includes the galaxies Messier 81 and Messier 82, as well as several other galaxies with high apparent brightnesses.<ref name="karachentsev2005">Template:Cite journal</ref> The approximate center of the group is located at a distance of 3.6 Mpc, making it one of the nearest groups to the Local Group.<ref name="karachentsev2005" /> The group is estimated to have a total mass of (1.03 ± 0.17)Template:ETemplate:Solar mass.<ref name="Karachentsevetal2006">Template:Cite journal</ref> The M81 Group, the Local Group, and other nearby groups all lie within the Virgo Supercluster (i.e. the Local Supercluster).<ref name="tully1982">Template:Cite journal</ref>
MembersEdit
Template:More references needed The table below lists galaxies that have been identified as associated with the M81 Group by I. D. Karachentsev.<ref name="karachentsev2005" />
Note that the object names used in the above table differ from the names used by Karachentsev. NGC, IC, UGC, and PGC numbers have been used in many cases to allow for easier referencing.
Interactions within the groupEdit
Messier 81, Messier 82, and NGC 3077 are all strongly interacting with each other.<ref name="yunetal1994">Template:Cite journal</ref> Observations of the 21-centimeter hydrogen line indicate how the galaxies are connected.<ref name="chynowethetal2008">Template:Cite journal</ref> The gravitational interactions have stripped some hydrogen gas away from all three galaxies, leading to the formation of filamentary gas structures within the group.<ref name="yunetal1994" /> Bridges of neutral hydrogen have been shown to connect M81 with M82 and NGC 3077.<ref name="chynowethetal2008" /><ref name="hulst1978">Template:Cite journal</ref> Moreover, the interactions have also caused some interstellar gas to fall into the centers of Messier 82 and NGC 3077, which has led to strong starburst activity (or the formation of many stars) within the centers of these two galaxies.<ref name="yunetal1994" /> Computer simulations of tidal interactions have been used to show how the current structure of the group could have been created.<ref name="yun1999">Template:Cite book</ref>
GalleryEdit
- The mysteries of UGC 8201.jpg
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- M81+M82-and other galaxies.jpg
Amateur picture Messier 81 + 82 and NGC 3077 all of the M81 group, 33 frames stacked of 1 minute each.
- M81m82 galex f.jpg
The spiral galaxies Messier 81 and 82 and the dwarf galaxy Holmberg IX from GALEX
- M81 wide Galex.jpg
Close up view of Messier 81 from GALEX
- Messier81 highres.jpg
The spiral galaxy Messier 81 from Spitzer Space Telescope
- Ssc2003-06c.jpg
The spiral galaxy Messier 81 from Spitzer Space Telescope
- M82 HST ACS 2006-14-a-large web.jpg
Starburst galaxy Messier 82 from Hubble Space Telescope
- NGC2403 3.6 5.8 8.0 microns spitzer.png
NGC 2403 in mid-infrared view, combining the 3.6, 5.8 and 8.0 μm bands of the Spitzer Space Telescope
- NGC2403 3.6 8.0 24 microns spitzer.png
NGC 2403 in Mid-infrared view, combining the 3.6, 8.0 and 24 μm bands of the Spitzer Space Telescope
- NGC 2403HST.jpg
NGC 2403 from Hubble Space Telescope
- NGC 2403HSTSN.jpg
NGC 2403 from Hubble Space Telescope illustrated
- Galaxy-NGC-2403-with-SN2004DJ.jpeg
Supernova SN2004DJ in the spiral galaxy NGC 2403
- NGC2403-SN2004dj.jpg
Supernova 2004dj in NGC 2403
- NGC 4236 I FUV g2006.jpg
NGC 4236 from GALEX
- NGC 2366HST.jpg
NGC 2366 from Hubble Space Telescope
- NGC 2976SSTFull.jpg
Galaxy NGC 2976 from Spitzer Space Telescope in infrared
- NGC2976.jpg
Galaxy NGC 2976 from an amateur Astronomer
- NGC 4605 GALEX WikiSky.jpg
Galaxy NGC 4605 from GALEX
- Ngc2363HST.jpg
NGC 2363 from Hubble Space Telescope
- NGC 2537 I FUV g2006.jpeg
NGC 2537 from GALEX
- Holmberg IISST.jpg
Holmberg II from Spitzer Space Telescope in infrared
- M81DwarBSST.jpg
UGC 5423 / M81 dwarf B from Spitzer Space Telescope in infrared
- NGC 3077 2MASS.jpg
NGC 3077 from 2MASS
- IC 2574 Hubble WikiSky.jpg
IC 2574