FINDING FOSSIL GROUPS: OPTICAL IDENTIFICATION AND X-RAY CONFIRMATION


Autoria(s): Miller, Eric D.; Rykoff, Eli S.; Dupke, Renato A.; de Oliveira, Claudia Mendes; de Oliveira, Raimundo Lopes; Proctor, Robert N.; Garmire, Gordon P.; Koester, Benjamin P.; McKay, Timothy A.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

05/11/2013

05/11/2013

2012

Resumo

We report the discovery of 12 new fossil groups (FGs) of galaxies, systems dominated by a single giant elliptical galaxy and cluster-scale gravitational potential, but lacking the population of bright galaxies typically seen in galaxy clusters. These FGs, selected from the maxBCG optical cluster catalog, were detected in snapshot observations with the Chandra X-ray Observatory. We detail the highly successful selection method, with an 80% success rate in identifying 12 FGs from our target sample of 15 candidates. For 11 of the systems, we determine the X-ray luminosity, temperature, and hydrostatic mass, which do not deviate significantly from expectations for normal systems, spanning a range typical of rich groups and poor clusters of galaxies. A small number of detected FGs are morphologically irregular, possibly due to past mergers, interaction of the intra-group medium with a central active galactic nucleus (AGN), or superposition of multiple massive halos. Two-thirds of the X-ray-detected FGs exhibit X-ray emission associated with the central brightest cluster galaxy (BCG), although we are unable to distinguish between AGN and extended thermal galaxy emission using the current data. This sample representing a large increase in the number of known FGs, will be invaluable for future planned observations to determine FG temperature, gas density, metal abundance, and mass distributions, and to compare to normal (non-fossil) systems. Finally, the presence of a population of galaxy-poor systems may bias mass function determinations that measure richness from galaxy counts. When used to constrain power spectrum normalization and Omega(m), these biased mass functions may in turn bias these results.

NASA through SAO [2834-MIT-SAO-4018]

NASA through SAO

NASA

NASA [NAS8-03060, NNH10CD19C]

Chandra Award [GO9-0142A]

Chandra Award

Brazilian agency FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo) [2009/06295-7, 2010/08341-3]

Brazilian agency Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP)

Chandra XRay Observatory Center

Chandra X-Ray Observatory Center

Identificador

ASTROPHYSICAL JOURNAL, BRISTOL, v. 747, n. 2, supl. 1, Part 6, pp. 132-151, 40238, 2012

0004-637X

http://www.producao.usp.br/handle/BDPI/41937

10.1088/0004-637X/747/2/94

http://dx.doi.org/10.1088/0004-637X/747/2/94

Idioma(s)

eng

Publicador

IOP PUBLISHING LTD

BRISTOL

Relação

ASTROPHYSICAL JOURNAL

Direitos

closedAccess

Copyright IOP PUBLISHING LTD

Palavras-Chave #GALAXIES: CLUSTERS: GENERAL #GALAXIES: CLUSTERS: INTRACLUSTER MEDIUM #GALAXIES: GROUPS: GENERAL #SURVEYS #X-RAYS: GALAXIES: CLUSTERS #DIGITAL SKY SURVEY #BRIGHTEST CLUSTER GALAXIES #SCALING RELATIONS #COSMOLOGICAL SIMULATIONS #STATISTICAL PROPERTIES #LUMINOSITY FUNCTIONS #VELOCITY DISPERSION #RICHNESS RELATION #HOST GALAXIES #RADIO-SOURCES #ASTRONOMY & ASTROPHYSICS
Tipo

article

original article

publishedVersion