EDP Sciences
Free Access
Volume 379, Number 1, November III 2001
Page(s) L1 - L4
Section Letters
DOI https://doi.org/10.1051/0004-6361:20011338
Published online 15 November 2001

A&A 379, L1-L4 (2001)
DOI: 10.1051/0004-6361:20011338

The dividing line between FR I and FR II radio-galaxies

G. Ghisellini1 and A. Celotti2

1  Osservatorio Astronomico di Brera, via Bianchi 46, 23807 Merate, Italy
2  SISSA/ISAS, via Beirut 2-4, 34014 Trieste, Italy

(Received 2 July 2001 / Accepted 18 July 2001 )

In the radio -host galaxy optical luminosity plane FR I and FR II radio-galaxies are clearly divided. Since the optical luminosity of an elliptical galaxy is an indication of the mass of its central black hole, we propose that the FR I-FR II dividing luminosity is a function of the mass of the black hole powering the active nucleus. Furthermore, as the radio power gives an estimate of the total kinetic power carried by the jet, the FR I-FR II separation can be re-interpreted as occurring at a constant ratio between the jet power and the black hole mass. There is also convincing evidence of a correlation between the radio power and the luminosity in narrow emission lines. As the latter results from photoionization by the radiation produced by accretion, we can estimate the ionizing luminosity and find that the separation luminosity can be also re-expressed as a constant accretion rate between ${\sim} 10^{-2}$-10-3 of the Eddington one. This possibly regulates the accretion mode and the consequent presence and characteristics of nuclear outflows.

Key words: galaxies: jets -- galaxies: nuclei -- radio continuum: galaxies

Offprint request: G. Ghisellini, gabriele@merate.mi.astro.it

© ESO 2001

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