Redshift-distance survey of early-type galaxies:: Spectroscopic data

被引:114
作者
Wegner, G [1 ]
Bernardi, M
Willmer, CNA
da Costa, LN
Alonso, MV
Pellegrini, PS
Maia, MAG
Chaves, OL
Rité, C
机构
[1] Dartmouth Coll, Dept Phys & Astron, Wilder Lab 6127, Hanover, NH 03755 USA
[2] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA
[3] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
[4] Observ Valongo, BR-20080090 Rio De Janeiro, Brazil
[5] Observ Nacl, BR-20921400 Rio De Janeiro, Brazil
[6] European So Observ, D-85748 Garching, Germany
[7] Observ Astron, RA-5000 Cordoba, Argentina
[8] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF, Argentina
[9] Observ Midi Pyrenees, Astrophys Lab, F-31400 Toulouse, France
关键词
galaxies : distances and redshifts; galaxies : elliptical and lenticular; cD; galaxies : general; large-scale structure of universe; surveys; techniques : spectroscopic;
D O I
10.1086/378959
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present central velocity dispersions and Mg-2 line indices for an all-sky sample of similar to1178 elliptical and S0 galaxies, of which 984 had no previous measures. This sample contains the largest set of homogeneous spectroscopic data for a uniform sample of elliptical galaxies in the nearby universe. These galaxies were observed as part of the ENEAR project, designed to study the peculiar motions and internal properties of the local early-type galaxies. Using 523 repeated observations of 317 galaxies obtained during different runs, the data are brought to a common zero point. These multiple observations, taken during the many runs and different instrumental setups employed for this project, are used to derive statistical corrections to the data and are found to be relatively small, typically less than or similar to5% of the velocity dispersion and 0.01 mag in the Mg-2 line strength. Typical errors are about 8% in velocity dispersion and 0.01 mag in Mg-2, in good agreement with values published elsewhere.
引用
收藏
页码:2268 / 2280
页数:13
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