- Canis Major Dwarf Galaxy
Infobox Galaxy
name = Canis Major Dwarf
epoch =J2000
type = Irr
ra = RA|07|12|35.0cite web
title=NASA/IPAC Extragalactic Database
work=Results for Canis Major Dwarf
url=http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=Canis+Major+Dwarf#ObjNo1
accessdate=2007-03-16]
dec = DEC|-27|40|00
dist_ly = 25,000 ly
z =
appmag_v =
size_v = 12 degrees × 12 degrees
constellation name =Canis Major
notes = -
names = CMa DwarfThe Canis Major Dwarf galaxy is located in the same part of the sky as the
constellation ofCanis Major . Thegalaxy contains a relatively high percentage ofred giant star s, and is thought to contain an estimated one billion stars in all.The Canis Major
dwarf galaxy is classified as anirregular galaxy and is now thought to be the closest neighbouring galaxy to our location in theMilky Way , being located about 25,000 light-years away from ourSolar System Fact|date=February 2007 and 42,000light-year s from theGalactic Center . It has a roughly elliptical shape and is thought to contain as many stars as theSagittarius Dwarf Elliptical Galaxy , the previous contender for closest galaxy to our location in the Milky Way.The galaxy was first discovered in November 2003 by an international team of French, Italian, British and Australian
astronomer s. Although closer to theEarth than the centre of the galaxy itself, the Canis Major Dwarf galaxy was difficult to detect as it is located behind the plane of the Milky Way, where concentrations of stars, gas and dust are densest. This, along with its small size, explains why it was not discovered sooner.The team of astronomers that discovered it were collaborating on analysis of data from the Two-Micron All Sky Survey (2MASS), a comprehensive survey of the sky in
infrared light, which is not blocked by gas and dust as severely as visible light. Because of this technique, scientists were able to detect a very significant over-density of class M giant stars in a part of the sky occupied by the Canis Major constellation, along with several other related structures composed of this type of star, two of which form broad, faint arcs.Astronomers believe that the Canis Major Dwarf Galaxy is in the process of being pulled apart by the
gravitational field of the more massive Milky Way galaxy. The main body of the galaxy is extremely degraded. Tidal disruption causes a long filament of stars to trail behind it as it orbits the Milky Way, forming a complex ringlike structure sometimes referred to as theMonoceros Ring which wraps around our galaxy three times. The stream of stars was first discovered in the early 21st century by astronomers conducting theSloan Digital Sky Survey . It was in the course of investigating this ring of stars, and a closely spaced group ofglobular clusters similar to those associated with the Sagittarius Dwarf Elliptical Galaxy, that the Canis Major dwarf galaxy was discovered.Globular clusters thought to be associated with the Canis Major Dwarf galaxy include
NGC 1851 ,NGC 1904 ,NGC 2298 andNGC 2808 , all of which are likely to be a remnant of the galaxy's globular cluster system before its "accretion", or swallowing, into the Milky Way.NGC 1261 is another nearby cluster, but its velocity is different enough from that of the others to make its relation to the system unclear. The Canis Major Dwarf galaxy may also have associatedopen cluster s, includingDol 25 andH18 , and possiblyAM-2 . It is thought that the open clusters may have formed due to the dwarf galaxy's gravity perturbing material in thegalactic disk and stimulatingstar formation .The discovery of the Canis Major Dwarf Galaxy and subsequent analysis of the stars associated with it has provided some support for the current theory that galaxies may grow in size by swallowing their smaller neighbors. Martin et al. believe that the preponderance of evidence points to the accretion of a small
satellite galaxy of the Milky Way which was orbiting roughly in the plane of thegalactic disk .A new study by
Yazan Momany using 2MASS data casts doubts on the nature of the dwarf galaxy. The data suggests that the trail of stars is actually part of the warped galactic disc. This conclusion, however, is still being challenged and the true nature of the overdensity inCanis Major remains unknown.Fact|date=June 2007ee also
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Messier 79
*Galaxy formation and evolution References
* N. F. Martin, R. A. Ibata, M. Bellazzini, M. J. Irwin, G. F. Lewis, W. Dehnen, (February 2004). [http://xxx.lanl.gov/abs/astro-ph/0311010 A dwarf galaxy remnant in Canis Major: the fossil of an in-plane accretion onto the Milky Way.] "Monthly Notices of the Royal Astronomical Society" 348 (1) 12.
* [http://astro.u-strasbg.fr/images_ri/canm-e.html Official press release announcing discovery (University of Strasbourg)]
* [http://www.seds.org/messier/more/cma_dw.html SEDS page on the Canis Major dwarf galaxy]External links
* [http://www.skynightly.com/reports/Deriving_The_Shape_Of_The_Galactic_Stellar_Disc.html Deriving The Shape Of The Galactic Stellar Disc] (SkyNightly) Mar 17, 2006
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