Fossil groups: end products of groups and clusters?

Computer Science

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Scientific paper

The prime objective of this program is to test the interesting possibility that a fossil group is the end-product of the merging of dense groups/poor clusters and to check if they are old systems, as commonly thought. Fossil groups, sometimes called ``dark" groups, exhibit an extended X-ray halo, with Lx, total mass and gas mass similar to poor clusters, but optically they are dominated by a single luminous elliptical galaxy, surrounded by faint companions. Our plan is to obtain a homogeneous spectroscopic and imaging dataset for all fossil groups known to date, complementing the X-ray studies. We will test the proposed evolutionary history through the determination of the luminosity function, velocity dispersions, total masses and M/L for a sample of 25 fossil groups and the detailed study of their first-ranked galaxies. In addition, the dataset will provide the basis for studies of galaxy populations, including analysis of the role of merging in the evolution of group members, and determination of the relationship of these groups with more typical groups and clusters.

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