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LCDM Satellites and HI Companions - The Arecibo ALFA Survey of NGC 2903 | | J. A. Irwin
; G. L. Hoffman
; K. Spekkens
; M. P. Haynes
; R. Giovanelli
; S. M. Linder
; B. Catinella
; E. Momjian
; B. S. Koribalski
; J. Davies
; E. Brinks
; W. J. G. de Blok
; M. E. Putman
; W. van Driel
; | | Date: |
7 Oct 2008 | | Abstract: | We have conducted a deep, complete HI survey, using Arecibo/ALFA, of a field
centered on the nearby, isolated galaxy, NGC 2903, which is similar to the
Milky Way in its properties. The field size was 150 kpc x 260 kpc and the final
velocity range spanned from 100 to 1133 km/s. The ALFA beams have been mapped
as a function of azimuth and cleaned from each azimuth-specific cube prior to
forming final cubes. The final HI data are sensitive down to an HI mass of 2 x
10^5 Mo and column density of 2 x 10^{17} cm^{-2} at the 3sigma x 2deltaV
level, where sigma is the rms noise level and deltaV is the velocity
resolution. NGC 2903 is found to have an HI envelope that is larger than
previously known, extending to at least 3 times the optical diameter of the
galaxy. Our search for companions yields one new discovery with an HI mass of
2.6 x 10^6 Mo. The companion is 64 kpc from NGC 2903 in projection, is likely
associated with a small optical galaxy of similar total stellar mass, and is
dark matter dominated, with a total mass >10^8 Mo. In the region surveyed,
there are now two known companions: our new discovery and a previously known
system that is likely a dwarf spheroidal, lacking HI content. If HI constitutes
1% of the total mass in all possible companions, then we should have detected
230 companions, according to LCDM predictions. Consequently, if this number of
dark matter clumps are indeed present, then they contain less than 1% HI
content, possibly existing as very faint dwarf spheroidals or as starless,
gasless dark matter clumps. | | Source: | arXiv, 0810.1090 | | Services: | Forum | Review | PDF | Favorites | |
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