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On the evolution of the black-hole : spheroid mass ratio

Abstract:

We present the results of a study which uses the 3CRR sample of radio-loud active galactic nuclei (AGN) to investigate the evolution of the black-hole:spheroid relation in the most massive early-type galaxies from 0 < z < 2. Radio-loud unification is exploited to obtain virial (line-width) black-hole mass estimates from the 3CRR quasars, and stellar mass estimates from the 3CRR radio galaxies, thereby providing black-hole and stellar mass estimates for a single population of early-type ...

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Publication status:
Published

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Publisher copy:
10.1016/j.newar.2006.06.010

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Volume:
50
Issue:
9-10
Pages:
782-785
Publication date:
2006-11-05
DOI:
ISSN:
1387-6473
URN:
uuid:1a18385b-6e60-4592-b86d-6f2e79fdae46
Source identifiers:
335090
Local pid:
pubs:335090

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