TY - JOUR
T1 - Fossil systems in the 400d cluster catalog
AU - Voevodkin, Alexey
AU - Borozdin, Konstantin
AU - Heitmann, Katrin
AU - Habib, Salman
AU - Vikhlinin, Alexey
AU - Mescheryakov, Alexander
AU - Hornstrup, Allan
AU - Burenin, Rodion
PY - 2010
Y1 - 2010
N2 - We report the discovery of seven new fossil systems in the 400d cluster survey. Our search targets nearby, z ≤ 0.2, and X-ray bright, LX ≥ 10^43 erg s-1, clusters of galaxies. Where available, we measure the optical luminosities from Sloan Digital Sky Survey images, thereby obtaining uniform sets of both X-ray and optical data. Our selection criteria identify 12 fossil systems, out of which five are known from previous studies. While in general agreement with earlier results, our larger sample size allows us to put tighter constraints on the number density of fossil clusters. It has been previously reported that fossil groups are more X-ray bright than other X-ray groups of galaxies for the same optical luminosity. We find, however, that the X-ray brightness of massive fossil systems is consistent with that of the general population of galaxy clusters and follows the same LX-Lopt scaling relation.
AB - We report the discovery of seven new fossil systems in the 400d cluster survey. Our search targets nearby, z ≤ 0.2, and X-ray bright, LX ≥ 10^43 erg s-1, clusters of galaxies. Where available, we measure the optical luminosities from Sloan Digital Sky Survey images, thereby obtaining uniform sets of both X-ray and optical data. Our selection criteria identify 12 fossil systems, out of which five are known from previous studies. While in general agreement with earlier results, our larger sample size allows us to put tighter constraints on the number density of fossil clusters. It has been previously reported that fossil groups are more X-ray bright than other X-ray groups of galaxies for the same optical luminosity. We find, however, that the X-ray brightness of massive fossil systems is consistent with that of the general population of galaxy clusters and follows the same LX-Lopt scaling relation.
U2 - 10.1088/0004-637X/708/2/1376
DO - 10.1088/0004-637X/708/2/1376
M3 - Journal article
SN - 0004-637X
VL - 708
SP - 1376
EP - 1387
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
ER -