REVISITING THE FOSSIL GROUP CANDIDATES UGC 842 AND NGC 6034


Autoria(s): OLIVEIRA, R. Lopes de; CARRASCO, E. R.; OLIVEIRA, C. Mendes de; BORTOLETTO, D. R.; CYPRIANO, E.; SODRE JR., L.; LIMA NETO, G. B.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

18/04/2012

18/04/2012

2010

Resumo

We present a new insight on NGC 6034 and UGC 842, two groups of galaxies previously reported in the literature as being fossil groups. The study is based on optical photometry and spectroscopy obtained with the CTIO Blanco telescope and Sloan Digital Sky Survey archival data. We find that NGC 6034 is embedded in a large structure, dominated by three rich clusters and other small groups. Its first and next four ranked galaxies have magnitude differences in the r band and projected distances which violate the optical criteria to classify it as a fossil group. We confirm that the UGC 842 group is a fossil group, but with about half the velocity dispersion that is reported in previous works. The velocity distribution of its galaxies reveals the existence of two structures in its line of sight, one with sigma(nu) similar to 223 km s(-1) and another with sigma(nu) similar to 235 km s(-1), with a difference in velocity of similar to 820 km s(-1). The main structure is dominated by passive galaxies, while these represent similar to 60% of the second structure. The X-ray temperature for the intragroup medium of a group with such a velocity dispersion is expected to be kT similar to 0.5-1 keV, against the observed value of kT similar to 1.9 keV reported in the literature. This result makes UGC 842 a special case among fossil groups because (1) it represents more likely the interaction between two small groups, which warms the intragroup medium and/or (2) it could constitute evidence that member galaxies lost energy in the process of spiraling toward the group center, and decreased the velocity dispersion of the system. As far as we know, UGC 842 is the first low-mass fossil group studied in detail.

Brazilian agency FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)[2007/04710-1]

CNPq (Conselho Nacional de Desenvolvimento Cientifico e Tecnologico)

Gemini Observatory

NASA National Aeronautics and Space Administration

Alfred P. Sloan Foundation

Participating Institutions

National Science Foundation (NSF)

U.S. Department of Energy (DOE)

Japanese Monbukagakusho (MEXT)

Max Planck Society

Higher Education Funding Council for England

Identificador

ASTRONOMICAL JOURNAL, v.139, n.1, p.216-227, 2010

0004-6256

http://producao.usp.br/handle/BDPI/15677

10.1088/0004-6256/139/1/216

http://dx.doi.org/10.1088/0004-6256/139/1/216

Idioma(s)

eng

Publicador

IOP PUBLISHING LTD

Relação

Astronomical Journal

Direitos

closedAccess

Copyright IOP PUBLISHING LTD

Palavras-Chave #cosmology: observations #galaxies: clusters: individual (UGC 842, NGC 6034) #galaxies: elliptical and lenticular, cD #galaxies: evolution #galaxies: kinematics and dynamics #intergalactic medium #DIGITAL SKY SURVEY #CFA REDSHIFT SURVEY #X-RAY #GALAXY GROUPS #MILLENNIUM SIMULATION #LUMINOSITY FUNCTION #HERCULES CLUSTER #DARK-MATTER #COMPILATION #GAS #Astronomy & Astrophysics
Tipo

article

original article

publishedVersion