2005A&A...431..517K

Query : 2005A&A...431..517K

2005A&A...431..517K - Astronomy and Astrophysics, volume 431, 517-521 (2005/2-4)

The great disk of Milky-Way satellites and cosmological sub-structures.

KROUPA P., THEIS C. and BOILY C.M.

Abstract (from CDS):

We show that the shape of the observed distribution of Milky Way (MW) satellites is inconsistent with their being drawn from a cosmological sub-structure population with a confidence of 99.5 per cent. Most of the MW satellites therefore cannot be related to dark-matter dominated satellites.

Abstract Copyright: ∼

Journal keyword(s): Galaxy: evolution - Galaxy: halo - galaxies: dwarf - galaxies: kinematics and dynamics - galaxies: Local Group - Galaxy: formation

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 11149 1
2 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 17434 0
3 Z 64-73 G 10 08 28.12 +12 18 23.4   11.3 10.0     ~ 1208 1
4 NAME UMi Galaxy G 15 09 08.0 +67 13 21   13.60 10.6     ~ 1360 0
5 NAME Dra dSph G 17 20 14.335 +57 55 16.39   12.40 10.6     ~ 1331 1
6 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 14415 0

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