Loose groups of galaxies in the Las Campanas Redshift Survey

被引:84
作者
Tucker, DL
Oemler, A
Hashimoto, Y
Shectman, SA
Kirshner, RP
Lin, H
Landy, SD
Schechter, PL
Allam, SS
机构
[1] Fermi Natl Accelerator Lab, Batavia, IL 60510 USA
[2] Carnegie Observ, Pasadena, CA 91101 USA
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[5] Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA
[6] MIT, Dept Phys, Cambridge, MA 02139 USA
[7] Helwan Observ, Natl Res Inst Astron & Geophys, Cairo, Egypt
[8] Yale Univ, Dept Astron, New Haven, CT 06520 USA
关键词
catalogs; galaxies : clusters : general; galaxies : distances and redshifts; large-scale structure of universe; surveys;
D O I
10.1086/317348
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A "friends-of-friends" percolation algorithm has been used to extract a catalog of deltan/n = 80 density enhancements (groups) from the six slices of the Las Campanas Redshift Survey (LCRS). The full catalog contains 1495 groups and includes 35% of the LCRS galaxy sample. A clean sample of 394 groups has been derived by culling groups from the full sample that either are too close to a slice edge, have a crossing time greater than a Hubble time, have a corrected velocity dispersion of zero, or contain a 55 " "orphan" (a galaxy with a mock redshift that was excluded from the original LCRS redshift catalog due to its proximity to another galaxy-i.e., within 55 "). Median properties derived from the clean sample include a line-of-sight velocity dispersion sigma (los) = 164 km s(-1), crossing time t(cr), = 0.10 H-0(-1), harmonic radius R-h = 0.58 h(-1) Mpc, pairwise separation R-p = 0.64 h(-1) Mpc, virial mass M-vir = 1.90 x 10(13) h(-1) M., total group R-band luminosity L-tot = 1.30 x 10(11) h(-2) L., and R-band mass-to-light ratio M/L = 171 h M./L.; the median number of observed members in a group is three.
引用
收藏
页码:237 / 265
页数:29
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