HI in Local Group analogs: What does it tell us about galaxy formation?

D. J. Pisano, D. G. Barnes, B. K. Gibson, Lister Staveley-Smith, K. C. Freeman, V. A. Kilborn

Research output: Chapter in Book/Report/Conference proceedingConference PaperResearchpeer-review

Abstract

We present the results of our HI survey of six loose groups of galaxies analogous to the Local Group. The survey was conducted using the Parkes telescope and the Australia Telescope Compact Array to produce a census of all the gas-rich galaxies and potential analogs to the high-velocity clouds (HVCs) within these groups down to MHI ≤ 107 M⊙ as a test of models of galaxy formation. We present the HI mass function and halo mass function for these analogous groups and compare them with the Local Group and other environments. We also demonstrate that our non-detection of HVC analogs in these groups implies that they must have low HI masses and be clustered tightly around galaxies, including around our own Milky Way, and are not distributed throughout the Local Group.

Original languageEnglish
Title of host publicationGroups of Galaxies in the Nearby Universe
Subtitle of host publicationProceedings of the ESO Workshop held at Santiago de Chile, December 5-9, 2005
EditorsIvo Saviane, Valentin Ivanov, Jordanka Borissova
Pages33-38
Number of pages6
DOIs
Publication statusPublished - 14 Aug 2007
Externally publishedYes

Publication series

NameESO Astrophysics Symposia
Volume2007
ISSN (Print)1431-2433
ISSN (Electronic)1611-6143

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