Optical Counterparts to Galaxies in the Cen A Group Discovered by HIPASS

Details Optical Counterparts to Galaxies in the Cen A Group Discovered by HIPASS Optical Counterparts to Galaxies in the Cen A Group Discovered by HIPASS

1999-05-10

arxiv.org/abs/astro-ph/9905114v1

Astronomy and Astrophysics

Astrophysics

8 pages, including 4 eps figures, to be published in PASA, vol. 16, in press

Scientific paper

We have completed a 21-cm survey of a 600 square degree region of the Centaurus A group of galaxies at a redshift of ~500 km/s as part of a larger survey of the entire southern sky. This group of galaxies was recently the subject of a separate and thorough optical survey (Cote et al. 1997), and thus presented an ideal comparison for us to test the survey performance. We have identified 10 new group members to add to the 21 already known in our survey area. Six of the new members are previously uncatalogued galaxies, while four were catalogued but assumed not to be group members. Including the 7 known members outside of our survey area, this brings the total known number of Cen A members to 38. All of the new HI detections have optical counterparts, most being intrinsically very faint (M(B) > -13.0), late-type low surface brightness dwarfs. Most of the new members have HI masses only a few times our survey limit of 10(7) M(solar) at an assumed distance for the group of 3.5 Mpc, and are extremely gas-rich, with a median M(HI)/L(B) > 1. Our limiting HI sensitivity was actually slightly worse than the HI follow-up observations of the Cote et al. optical survey, yet we have already increased the known number of group members by 50% using an HI survey technique. While we have increased the known NUMBER of members by ~50%, these new members contribute < 4% to its light.

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