The radio galaxy K-z relation: The 1012 M○. mass limit: Masses of galaxies from the LK luminosity, up to z > 4

• Published in: Astronomy and astrophysics (Berlin) 2004, Vol.415 (3), p.931-940
• Main Authors: ROCCA-VOLMERANGE, B, LE BORGNE, D, DE BREUCK, C, FIOC, M, MOY, E
• Format: Article
• Language: English
• Subjects: Sciences of the Universe
• ISSN: 0004-6361; 1432-0746; 1432-0756
• DOI: 10.1051/0004-6361:20031717

The narrow K-z relation of powerful radio galaxies in the Hubble K-band diagram is often attributed to the stellar populations of massive elliptical galaxies. Because it extends over a large range of redshifts (0 < z < 4), it is difficult to estimate masses at high redshifts by taking into account galaxy evolution. In the present paper, we propose to estimate the stellar masses of galaxies using the galaxy evolution model PÉGASE. We use star formation scenarios that successfully fit faint galaxy counts as well as z = 0 galaxy templates. These scenarios also predict spectra at higher z, used to estimate valid photometric redshifts. The baryonic mass of the initial gas cloud Mbar is then derived. The K-z relation is remarkably reproduced by our evolutionary scenario for elliptical galaxies of baryonic mass Mbar,max ≃ 1012 M⊙, at all z up to z = 4. Mbar,max is also the maximum mass limit of all types of galaxies. Using another initial mass function (IMF), even a top-heavy one, does not alter our conclusions. The high value of Mbar,max observed at z > 4 implies that massive clouds were already formed at early epochs. We also find that the Mbar,max limit is similar to the critical mass Mcrit of a self-gravitating cloud regulated by cooling (Rees & Ostriker \cite{Ree77}; Silk \cite{Sil77}). Moreover, the critical size rcrit≃ 75 kpc is remarkably close to the typical diameter of Lyα haloes surrounding distant radio galaxies. This confirms the validity of the method of baryonic mass determination based on the K-band luminosity. A puzzling question that remains to be answered is the short time-scale of mass-accumulation required to form such massive galaxies at z = 4. We discuss the dispersion of the K-z relation in terms of uncertainties on the mass limit. The link between the presence of the active nucleus and a large stellar mass is also discussed.