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2011MNRAS.410.1360H - Mon. Not. R. Astron. Soc., 410, 1360-1376 (2011/January-2)
The evolution of the fundamental plane of radio galaxies from z∼ 0.5 to the present day.
HERBERT P.D., JARVIS M.J., WILLOTT C.J., McLURE R.J., MITCHELL E., RAWLINGS S., HILL G.J. and DUNLOP J.S.
Abstract (from CDS):
We also find evidence for a correlation between host galaxy velocity dispersion and radio luminosity at the 97 per cent significance level within our subsample, although further observations are required in order to determine whether this is different for the FRI and FRII radio sources. Assuming that the MBH-σ relation still holds at z ∼ 0.5, this implies that radio luminosity scales with black hole mass, in agreement with previous studies.
Abstract Copyright: 2010 The Authors. Journal compilation2010 RAS
Journal keyword(s): galaxies: active - galaxies: fundamental parameters - galaxies: nuclei
Simbad objects: 30
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