期刊
ASTRONOMICAL JOURNAL
卷 145, 期 5, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/145/5/120
关键词
galaxies: evolution; galaxies: formation; galaxies: interactions; galaxies: kinematics and dynamics; large-scale structure of universe; radio lines: galaxies
资金
- National Science Foundation [1009476]
- University of Michigan
- Dartmouth College
- Ohio State University
- Columbia University
- Ohio University
- Netherlands Foundation
- INSU/CNRS (France)
- MPG (Germany)
- European Community's Seventh Framework Programme
- ASTRON (Netherlands Institute for Radio Astronomy)
- Da Vinci Professorship at the Kapteyn Institute
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1009476] Funding Source: National Science Foundation
Cosmological voids provide a unique environment for the study of galaxy formation and evolution. The galaxy population in their interiors has properties significantly different from average field galaxies. As part of our Void Galaxy Survey (VGS), we have found a system of three interacting galaxies (VGS_31) inside a large void. VGS_31 is a small elongated group whose members are embedded in a common Hi envelope. The Hi picture suggests a filamentary structure with accretion of intergalactic cold gas from the filament onto the galaxies. We present deep optical and narrowband H alpha data, optical spectroscopy, near-UV, and far-UV Galaxy Evolution Explorer and CO(1-0) data. We find that one of the galaxies, a Markarian object, has a ring-like structure and a tail evident both in optical and Hi. While all three galaxies form stars in their central parts, the tail and the ring of the Markarian object are devoid of star formation. We discuss these findings in terms of a gravitational interaction and ongoing growth of galaxies out of a filament. VGS_31 is one of the first observed examples of a filamentary structure in a void. It is an important prototype for understanding the formation of substructure in a void. This system also shows that the galaxy evolution in voids can be as dynamic as in high-density environments.
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