高红移团簇星系 K 带光度函数
天体物理学
2009-11-10 v1
摘要
presented. The evolution of K*, the characteristic magnitude of the LF, is consistent with purely passive evolution, and a redshift of formation z = 1.5-2.
引用
@article{arxiv.astro-ph/0405043,
title = {The K Band Luminosity Functions of Galaxies in High Redshift Clusters},
author = {S. C. Ellis and L. R. Jones},
journal= {arXiv preprint arXiv:astro-ph/0405043},
year = {2009}
}
备注
3 pages, to appear in Proceedings of IAU Colloquium 195 - Outskirts of Galaxy Clusters: intense life in the suburbs