Abstract
The fraction of galaxies bound in groups in the nearby Universe is high (50% at z~0). Systematic studies of galaxy properties in groups are important in order to improve our understanding of the evolution of galaxies and of the physical phenomena occurring within this environment. We have built a complete spectrophotometric sample of galaxies within X-ray detected, optically spectroscopically confirmed groups and clusters (G
Original language | English |
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Journal | Astronomy and Astrophysics |
Early online date | 6 Nov 2017 |
DOIs | |
Publication status | E-pub ahead of print - 6 Nov 2017 |
Bibliographical note
20 pages, 18 figures, 6 tables, accepted for publication in Astronomy & AstrophysicsKeywords
- astro-ph.GA
- 85A04