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(Referência obtida automaticamente do Google Scholar, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

Star formation efficiency in galaxy clusters

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Autor(es):
Laganá‚ TF ; Lima Neto‚ GB ; Andrade-Santos‚ F. ; Cypriano‚ ES
Número total de Autores: 4
Tipo de documento: Artigo Científico
Fonte: Astronomy & Astrophysics; v. 485, n. 3, p. 633-644, 2008.
Resumo

Context. The luminous material in clusters of galaxies exists in two forms: the visible galaxies and the X-ray emitting intra-cluster medium. The hot intra-cluster gas is the major observed baryonic component of clusters, about six times more massive than the stellar component. The mass contained within visible galaxies is approximately 3% of the dynamical mass. Aims. Our aim was to analyze both baryonic components, combining X-ray and optical data of a sample of five galaxy clusters (Abell 496, 1689, 2050, 2631 and 2667), within the redshift range 0.03 < z < 0.3. We determined the contribution of stars in galaxies and the intra-cluster medium to the total baryon budget. Methods. We used public XMM-Newton data to determine the gas mass and to obtain the X-ray substructures. Using the optical counterparts from SDSS or CFHT we determined the stellar contribution. Results. We examine the relative contribution of galaxies, intra-cluster light and intra-cluster medium to baryon budget in clusters through the stellar-to-gas mass ratio, estimated with recent data. We find that the stellar-to-gas mass ratio within r(500) (the radius within which the mean cluster density exceeds the critical density by a factor of 500), is anti-correlated with the ICM temperature, which range from 24% to 6% while the temperature ranges from 4.0 to 8.3 keV. This indicates that less massive cold clusters are more prolific star forming environments than massive hot clusters. (AU)

Processo FAPESP: 03/10345-3 - Matéria escura e bárions em aglomerado de galáxias: evolução e conversão em estrelas do gás intra-aglomerado
Beneficiário:Tatiana Ferraz Laganá
Modalidade de apoio: Bolsas no Brasil - Doutorado Direto
Processo FAPESP: 01/07342-7 - Evolução de galáxias em grupos e em aglomerados
Beneficiário:Claudia Lucia Mendes de Oliveira
Modalidade de apoio: Auxílio à Pesquisa - Temático