English

Radio luminosity function of brightest cluster galaxies

Astrophysics of Galaxies 2016-05-12 v1

Abstract

By cross-matching the currently largest optical catalog of galaxy clusters and the NVSS radio survey database, we obtain the largest complete sample of brightest cluster galaxies (BCGs) in the redshift range of 0.05<z<0.45, which have radio emission and redshift information. We confirm that more powerful radio BCGs tend to be these optically very bight galaxies located in more relaxed clusters. We derived the radio luminosity functions of BCGs from the largest complete sample of BCGs, and find that the functions depend on the optical luminosity of BCGs and the dynamical state of galaxy clusters. However, the radio luminosity function does not show significant evolution with redshift.

Keywords

Cite

@article{arxiv.1605.03387,
  title  = {Radio luminosity function of brightest cluster galaxies},
  author = {Z. S. Yuan and J. L. Han and Z. L. Wen},
  journal= {arXiv preprint arXiv:1605.03387},
  year   = {2016}
}

Comments

10 pages, 9 figures. MNRAS in press

R2 v1 2026-06-22T13:58:21.181Z