Astron. Astrophys. Suppl. Ser. 139, 1-24
Trinh X. Thuan13 - V.A. Lipovetsky2 - J.-M. Martin4 - S.A. Pustilnik2
request: Trinh X. Thuan
Deceased 1996 September 22.
1 - Astronomy
Department, University of Virginia, Charlottesville, VA 22903,
2 - Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Karachai-Circessia 357147, Russia
3 - Département d'Astronomie Extragalactique et de Cosmologie, Observatoire de Paris, F-92195 Meudon Cedex, France
4 - Département de Radioastronomie ARPEGES, Observatoire de Paris, F-92195 Meudon Cedex, France
Received August 11; accepted November 24, 1998
We present the results of a neutral hydrogen survey of 79 galaxies from a statistical sample of 88 Blue Compact Galaxies (BCGs) selected from the First and Second Byurakan objective prism surveys to have a HII region-like spectrum, an equivalent width of the [O III] line larger than , and a velocity km s-1. The detection rate for the statistical sample is 74%. HI masses range between and with the HI mass distribution peaking at . The full width at half-maximum of the HI profile varies between km s-1 and 160 km s-1, with a mean of 92 km s-1. These small widths are characteristic of dwarf galaxies. For comparison, we have also observed an additional 92 BCGs with weaker star formation and/or larger distances, and/or interesting astrophysical properties. These in general have larger widths and HI masses.
Key words: galaxies:
compact -- galaxies: ism -- galaxies: startburst -- radio lines:
galaxies -- radio lines: ISM