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Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-54812

Busha, M T; Wechsler, R H; Behroozi, P S; Gerke, B F; Klypin, A A; Primack, J R (2011). Statistics of Satellite Galaxies around Milky-Way-like hosts. Astrophysical Journal, 743(2):117.

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Abstract

We calculate the probability that a Milky-Way (MW)-like halo in the standard cosmological model has the observed number of Magellanic Clouds (MCs). The statistics of the number of MCs in the lambda cold dark matter model are in good agreement with observations of a large sample of Sloan Digital Sky Survey (SDSS) galaxies. Under the subhalo abundance matching assumption of a relationship with small scatter between galaxy r-band luminosities and halo internal velocities v max, we make detailed comparisons to similar measurements using SDSS Data Release 7 data by Liu et al. Models and observational data give very similar probabilities for having zero, one, and two MC-like satellites. In both cases, MW luminosity hosts have just a ~10% chance of hosting two satellites similar to the MCs. In addition, we present a prediction for the probability for a host galaxy to have N sats satellite galaxies as a function of the magnitudes of both the host and satellite. This probability and its scaling with host properties is significantly different from that of mass-selected objects because of scatter in the mass-luminosity relation and because of variations in the star formation efficiency with halo mass.

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
DDC:530 Physics
Language:English
Date:December 2011
Deposited On:18 Feb 2012 09:27
Last Modified:07 Jun 2014 02:30
Publisher:IOP Publishing
ISSN:0004-637X (P) 1538-4357 (E)
Publisher DOI:10.1088/0004-637X/743/2/117
Related URLs:http://arxiv.org/abs/1011.6373
Citations:Web of Science®. Times Cited: 33
Google Scholar™
Scopus®. Citation Count: 23

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