HI Deficiency Estimates in Galaxy Group WBL 368

Details HI Deficiency Estimates in Galaxy Group WBL 368 HI Deficiency Estimates in Galaxy Group WBL 368

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21840814h&link_type=abstract

American Astronomical Society, AAS Meeting #218, #408.14; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The Undergraduate ALFALFA (Arecibo Legacy Fast ALFA) Team Groups Project is a collaborative undertaking of faculty and undergraduates at 18 institutions, aimed at investigating properties of galaxy groups surveyed by the ALFALFA blind HI survey. The Hartwick College team is analyzing a 6X6 degree region centered on the galaxy group WBL 368. Using a new determination of group membership, we find the most probable optical counterparts for HI source detections of member galaxies. These detections are used to calculate the HI deficiencies in the group by comparing to a sample of HI field galaxies. This work has been supported by NSF grants AST-0724918, AST-0725267 and AST-0725380.

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