An HI Survey of Six Local Group Analogs. II. HI properties of group galaxies

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

70 pages, 35 figures, ApJ Supplement, in press

Scientific paper

We have conducted an HI 21 cm emission-line survey of six loose groups of galaxies chosen to be analogs to the Local Group. The survey was conducted using the Parkes Multibeam instrument and the Australia Telescope Compact Array (ATCA) over a ~1 Mpc^2 area and covering the full depth of each group, with a M(HI) sensitivity of ~7x10^5 M(sun). Our survey detected 110 sources, 61 of which are associated with the six groups. All of these sources were confirmed with ATCA observations or were previously cataloged by HIPASS. The sources all have optical counterparts and properties consistent with dwarf irregular or late-type spiral galaxies. We present here the HI properties of the groups and their galaxies. We derive an HI mass function for the groups that is consistent with being flatter than the equivalent field HIMF. We also derive a circular velocity distribution function, tracing the luminous dark matter halos in the groups, that is consistent with those of the Local Group and HIPASS galaxies, both of which are shallower than that of clusters or predictions from CDM models of galaxy formation.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

An HI Survey of Six Local Group Analogs. II. HI properties of group galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with An HI Survey of Six Local Group Analogs. II. HI properties of group galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An HI Survey of Six Local Group Analogs. II. HI properties of group galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-688043

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.