Luminosity and mass segregation of galaxies in groups

Details Luminosity and mass segregation of galaxies in groups Luminosity and mass segregation of galaxies in groups

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995astl...21..429m&link_type=abstract

Astronomy Letters, Volume 21, Issue 4, July 1995, pp.429-430; Pis'ma v Astronomicheskii Zhurnal, Vol. 21, p. 483

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Groups of galaxies are analyzed to reveal the segregation of galaxies of various luminosities and masses in their positions relative to the group centers and peculiar velocities within the groups. It is found that the brightest and most massive galaxies are, on average, closer to the group center, while the faintest and least massive galaxies are farther than galaxies with intermediate masses and luminosities. The segregation of galaxies of various luminosities and masses in their mean peculiar radial velocities is less pronounced.

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