Мақола

Evolution of red-sequence cluster galaxies from redshift 0.8 to 0.4: ages, metallicities, and morphologies

P. Sánchez–BlázquezCenter for Astrophysics, University of Central Lancashire, Preston, PR1 2HE, UK e-mail: [email protected]P. JablonkaGEPI, CNRS-UMR8111, Observatoire de Paris, section de Meudon, 5 Place Jules Janssen, 92195 Meudon Cedex, FranceStefan NollMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching bei München, GermanyBianca M. PoggiantiOsservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, ItalyJohn MoustakasCenter for Cosmology and Particle Physics, New York University, 4 Washington Place, New York, NY 10003, USAB. Milvang‐JensenDark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, DenmarkC. HallidayINAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, ItalyAlfonso Aragón-SalamancaSchool of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD, UKR. P. SagliaMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching bei München, GermanyVandana DesaiScience Center, Caltech, Pasadena CA 91125, USAG. De LuciaMax-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching bei München, GermanyDouglas CloweOhio University, Department of Physics and Astronomy, Clippinger Labs 251B, Athens, OH 45701, USAR. PellóLaboratoire d'Astrophysique de Toulouse-Tarbes, CNRS, Université de Toulouse, 14 Avenue Edouard Belin, 31400 Toulouse, FranceGregory RudnickL. SimardHerzberg Institute of Astrophysics, National Research Council of Canada, 5071 West Saanich Road, Victoria, Canada BC V9E 2E7, CanadaSimon D. M. WhiteMax-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching bei München, GermanyDennis ZaritskySteward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA

2009en

ABI

Аннотация

We present a comprehensive analysis of the stellar population properties and morphologies of red-sequence galaxies in 24 clusters and groups from to . The dataset, consisting of 215 spectra drawn from the ESO Distant Cluster Survey, constitutes the largest spectroscopic sample at these redshifts for which such an analysis has been conducted. Analysis reveals that the evolution of the stellar population properties of red-sequence galaxies depend on their mass: while the properties of the most massive are well described by passive evolution and high-redshift formation, those of the less massive galaxies are consistent with a more extended star-formation history. We show that these scenarios reproduce the index-σ relations and the galaxy colours. The two main results of this work are: (1) the evolution of the line-strength indices for the red-sequence galaxies can be reproduced if 40% of the galaxies with km s-1 entered the red-sequence between to , in agreement with the fraction derived in studies of the luminosity functions; and (2) the percentage of red-sequence galaxies exhibiting early-type morphologies (E and S0) decreases by 20% from to . This can be understood if the red-sequence becomes more populated at later times with disc galaxies whose star formation has been quenched. We conclude that the processes quenching star formation do not necessarily produce a simultaneous morphological transformation of the galaxies entering the red-sequence.

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Идентификаторлар

DOI: 10.1051/0004-6361/200811355

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