Fossil group origins - VI. Global X-ray scaling relations of fossil galaxy clusters
arXiv:1503.06219 · doi:10.1093/mnras/stv1879
Abstract
We present the first pointed X-ray observations of 10 candidate fossil galaxy groups and clusters. With these Suzaku observations, we determine global temperatures and bolometric X-ray luminosities of the intracluster medium (ICM) out to for six systems in our sample. The remaining four systems show signs of significant contamination from non-ICM sources. For the six objects with successfully determined properties, we measure global temperatures in the range , bolometric X-ray luminosities of , and estimate masses, as derived from , of . Fossil cluster scaling relations are constructed for a sample that combines our Suzaku observed fossils with fossils in the literature. Using measurements of global X-ray luminosity, temperature, optical luminosity, and velocity dispersion, scaling relations for the fossil sample are then compared with a control sample of non-fossil systems. We find the fits of our fossil cluster scaling relations are consistent with the relations for normal groups and clusters, indicating fossil clusters have global ICM X-ray properties similar to those of comparable mass non-fossil systems.
17 pages, 7 figures, 8 tables. Accepted for publication in MNRAS
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