Abstract
We examine the H I content of spiral galaxies in groups by using a catalog of loose groups of galaxies identified in a magnitude-limited sample (mz ≤ 15.7) spanning the range 8h ≤ α ≤ 18h in right ascension and +9° ≤ δ ≤ +15° in declination. The redshift completeness of the galaxy sample is approximately 95%. No significant effect of H I depletion is found, although there may be a hint that the earliest type spirals are slightly deficient.
Original language | English (US) |
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Pages (from-to) | 49-54 |
Number of pages | 6 |
Journal | Astronomical Journal |
Volume | 115 |
Issue number | 1 |
DOIs | |
State | Published - Jan 1998 |
Externally published | Yes |
Keywords
- Galaxies: clusters: general
- ISM: atoms
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science