Stellar mass-halo mass relation for the brightest central galaxies of X-ray clusters since z ~ 0.65 (2019)

First Author: Erfanianfar G

Attributed to: Quota Studentships funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201935375

Publication URI: http://dx.doi.org/10.1051/0004-6361/201935375

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics