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The Void Galaxy Survey

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arxiv 1101.4187 v1 pith:LKY5NED5 submitted 2011-01-21 astro-ph.CO

R. van de Weygaert , K. Kreckel , E. Platen , B. Beygu , J.H. van Gorkom , J.M. van der Hulst , M.A. Aragon-Calvo , P.J.E. Peebles
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T. Jarrett G. Rhee K. Kovac C.-W. Yip
This is my paper · ORCID
classification astro-ph.CO
keywords voidgalaxiesgalaxysurveyamongstcontentsampleaccretion
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abstract

The Void Galaxy Survey (VGS) is a multi-wavelength program to study $\sim$60 void galaxies. Each has been selected from the deepest interior regions of identified voids in the SDSS redshift survey on the basis of a unique geometric technique, with no a prior selection of intrinsic properties of the void galaxies. The project intends to study in detail the gas content, star formation history and stellar content, as well as kinematics and dynamics of void galaxies and their companions in a broad sample of void environments. It involves the HI imaging of the gas distribution in each of the VGS galaxies. Amongst its most tantalizing findings is the possible evidence for cold gas accretion in some of the most interesting objects, amongst which are a polar ring galaxy and a filamentary configuration of void galaxies. Here we shortly describe the scope of the VGS and the results of the full analysis of the pilot sample of 15 void galaxies.

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Cited by 1 Pith paper

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  1. The size of the HI disk across different environments: isolated, compact groups, clusters, and pairs

    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    Compact-group galaxies have HI disks at least ~71% smaller than isolated galaxies of the same optical size, with truncation increasing along the group evolutionary sequence.

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