HI Deficiency as a Function of Galaxy Type in the MKW11 Group

Details HI Deficiency as a Function of Galaxy Type in the MKW11 Group HI Deficiency as a Function of Galaxy Type in the MKW11 Group

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21714929t&link_type=abstract

American Astronomical Society, AAS Meeting #217, #149.29; 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 11 institutions, aimed at investigating properties of galaxy groups surveyed by the ALFALFA blind HI survey. As part of this project we examine a 10x10 degree region around the rich galaxy group MKW 11 in order to study HI deficiency as a function of local density as well as optical galaxy morphology. Our sample includes 496 galaxies in the Sloan Digital Sky Survey, 153 of which are detected in HI. This work has been supported by NSF grants AST-0724918, AST-0725267, and AST-0725380.

Affiliated with

Also associated with

No associations

Rating

HI Deficiency as a Function of Galaxy Type in the MKW11 Group 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 HI Deficiency as a Function of Galaxy Type in the MKW11 Group, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HI Deficiency as a Function of Galaxy Type in the MKW11 Group will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1395680