On the Nature of Fossil Galaxy Groups: Are they really fossils ?
F. La Barbera, R. R. de Carvalho, I. G. de la Rosa, G. Sorrentino, R., R. Gal, J. L. Kohl-Moreira

TL;DR
This study analyzes fossil galaxy groups using SDSS and ROSAT data, finding they are not distinct from regular ellipticals and may simply be the end stage of galaxy mass assembly.
Contribution
It provides a comprehensive comparison between fossil groups and field ellipticals, challenging the idea that fossils are a unique, ancient class of galaxy.
Findings
FGs have similar stellar populations to field ellipticals.
No significant differences in structural parameters between FGs and ellipticals.
FGs are likely not a distinct class but the end stage of galaxy assembly.
Abstract
We use SDSS-DR4 photometric and spectroscopic data out to redshift z~0.1 combined with ROSAT All Sky Survey X-ray data to produce a sample of twenty-five fossil groups (FGs), defined as bound systems dominated by a single, luminous elliptical galaxy with extended X-ray emission. We examine possible biases introduced by varying the parameters used to define the sample and the main pitfalls are discussed. The spatial density of FGs, estimated via the V/V_ MAX} test, is 2.83 x 10^{-6} h_{75}^3 Mpc^{-3} for L_x > 0.89 x 10^42 h_{75}^-2 erg/s consistent with Vikhlinin et al. (1999), who examined an X-ray overluminous elliptical galaxy sample (OLEG). We compare the general properties of FGs identified here with a sample of bright field ellipticals generated from the same dataset. These two samples show no differences in the distribution of neighboring faint galaxy density excess, distance…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies
