
A long-term program based on Fabry-Perot Ha velocity field data of compact groups has been undertaken in order to analyse the kinematics of the compact group galaxies and the extent of their dark halos. The data are taken at the ESO and the CFH 3.6 m telescopes. The main goals of our project are: To determine the evolutionary stages of the studied groups, To search for tidal dwarf galaxy candidates in heavily interacting systems and in combination with photometry available in the literature, to determine the Tully-Fisher relation for the group galaxies.
[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
| citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 7 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
