Group Membership and HI Sources in the WBL 368 Galaxy Group

Astronomy and Astrophysics – Astronomy

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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 around the galaxy group WBL 368, which has an average recessional velocity of 4732 km/s. Preliminary analysis using ALFALFA data and the Sloan Digital Sky Survey indicates a significant increase in group membership, with 47% of the member galaxies detected as HI sources. This work has been supported by NSF grants AST-0724918, AST-0725267 and AST-0725380.

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