By Rob Fender, Tomaso Belloni, Elena Gallo (auth.), T. J. Maccarone, R. P. Fender, L. C. Ho (eds.)
This quantity brings jointly contributions from some of the world's best professionals on black gap accretion. The papers inside symbolize a part of a brand new flow to use the relative benefits of learning stellar mass and supermassive black holes and to collect the information received from the 2 methods. the subjects mentioned the following run the gamut of the state-of-the-art in black gap observational and theoretical work-variability, spectroscopy, disk-jet connections, and multi-wavelength campaigns on black holes are all covered.
Reprinted from ASTROPHYSICS AND house technology, 300:1-3 (2005)
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Additional info for Astrophysics and Space Science: From X-Ray Binaries to Quasars: Black Holes on all Mass Scales
1984, Rev. Mod. Phys. 56, 255. Falcke, H. : 1995, A&A 293, 665. , K¨ording, E. : 2004, A&A 414, 895. , Gallo, E. : 2003, MNRAS 343, L99. , Belloni, T. : 2004, MNRAS in press, astro-ph/0409360. : 1998, MNRAS 297, 817. P. : 2003, MNRAS 344, 60. Heinz, S. : 2003, MNRAS 343, L59. : 2004, to appear in the Proceedings of ‘Growing Black Holes’, Garching, Germany, June 21–25, 2004. A. Merloni, S. Nayakshin and R. ), Springer-Verlag series of ‘ESO Astrophysics Symposia’. : 2002, ApJ 564, 120. C. : 2001, ApJ 555, 650.
1). The low m˙ ‘peak’ comprises low excitation narrow line RG, LINERs and some low ionization Seyfert 2. The similarity found between the behavior of radio-loud and radio-quiet sources, spanning a different range of BH masses and having different host galaxies, thus suggests that such bimodal transition might indeed occur in all accreting systems. As brieﬂy discussed in Marchesini et al. (2004) and Ballo and Celotti (2005), one can envisage different processes leading to such a distribution and in particular to a transition and a gap in the luminosity/inferred accretion rate.
We therefore excluded from our sample BL Lac objects. Among the Quasars in our sample, only 3C 273, which has an extremely high radio loudness and a blazar-like spectrum, is likely to suffer from strong Doppler boosting of the radio jet. On the other hand, according to the uniﬁcation scheme, Seyfert 2 nuclei should not be preferentially viewed pole on, while for all the other sources (mainly low-luminosity AGN and Seyfert 1), for which the nature of the (relatively faint) radio emission is not well established, we have assumed that the orientation of their jets with respect to line of sight is randomly distributed.
Astrophysics and Space Science: From X-Ray Binaries to Quasars: Black Holes on all Mass Scales by Rob Fender, Tomaso Belloni, Elena Gallo (auth.), T. J. Maccarone, R. P. Fender, L. C. Ho (eds.)