3 research outputs found
Black Hole Spin Properties of 130 AGN
Supermassive black holes may be described by their mass and spin. When
supermassive black holes are active, the activity provides a probe of the state
of the black hole system. The spin of a hole can be estimated when the black
hole mass and beam power of the source are known for sources with powerful
outflows. Seventy-five sources for which both the black hole mass and beam
power could be obtained are identified and used to obtain estimates of black
hole spins. The 75 supermassive black holes studied include 52 FRII radio
galaxies and 23 FRII radio loud quasars with redshifts ranging from about zero
to two. The new values are combined with those obtained previously for 19 FRII
radio galaxies, 7 FRII radio loud quasars, and 29 radio sources associated with
CD galaxies to form samples of 71 FRII radio galaxies, 30 FRII quasars, and a
total sample of 130 spin values; all of the sources are associated with massive
elliptical galaxies. The new values obtained are similar to those obtained
earlier at similar redshift, and range from about 0.1 to 1 for FRII sources.
The overall results are consistent with those obtained previously: the spins
tend to decrease with decreasing redshift for the FRII sources studied. There
is a hint that the range of values of black hole spin at a given redshift is
larger for FRII quasars than for FRII radio galaxies. There is no indication of
a strong correlation between supermassive black hole mass and spin for the
supermassive black holes studied here. The relation between beam power and
black hole mass is obtained and used as a diagnostic of the outflows and the
dependence of the magnetic field strength on black hole mass.Comment: 12 pages, 12 figures, 5 table
The Relationship Between Beam Power and Radio Power for Classical Double Radio Sources
Beam power is a fundamental parameter that describes, in part, the state of a
supermassive black hole system. Determining the beam powers of powerful
classical double radio sources requires substantial observing time, so it would
be useful to determine the relationship between beam power and radio power so
that radio power could be used as a proxy for beam power. A sample of 31
powerful classical double radio sources with previously determined beam and
radio powers are studied; the sources have redshifts between about 0.056 and
1.8. It is found that the relationship between beam power, Lj, and radio power,
P, is well described by Log(Lj) = 0.84 Log(P) + 2.15, where both L_j and P are
in units of 10^(44) erg/s. This indicates that beam power is converted to radio
power with an efficiency of about 0.7%. The ratio of beam power to radio power
is studied as a function of redshift; there is no significant evidence for
redshift evolution of this ratio over the redshift range studied. The
relationship is consistent with empirical results obtained by Cavagnolo et al.
(2010) for radio sources in gas rich environments, which are primarily FRI
sources, and with the theoretical predictions of Willott et al. (1999).Comment: 6 pages, 2 figures, 2 tables; accepted for publication in MNRA