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Brightest group galaxies โ II: the relative contribution of BGGs to the total baryon content of groups at z < 1.3
We performed a detailed study of the evolution of the star formation rate (SFR) and stellar mass of the brightest group galaxies (BGGs) and their relative contribution to the total baryon budget within R200 (โ |$f^{{\rm BGG}}_{{\rm b},200}$|โ ). The sample comprises 407 BGGs selected from X-ray groups (M200 = 1012.8โ1014 Mโ) โฆ