期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 343, 期 3, 页码 L59-L64出版社
BLACKWELL PUBLISHING LTD
DOI: 10.1046/j.1365-8711.2003.06918.x
关键词
radiation mechanisms : non-thermal; galaxies : active; galaxies : jets; galaxies : nuclei; radio continuum : general; X-rays : binaries
We derive the non-linear relation between the core flux F (nu) of accretion-powered jets at a given frequency and the mass M of the central compact object. For scale-invariant jet models, the mathematical structure of the equations describing the synchrotron emission from jets enables us to cancel out the model-dependent complications of jet dynamics, retaining only a simple, model-independent algebraic relation between F-nu and M . This approach allows us to derive the F-nu -M relation for any accretion disc scenario that provides a set of input boundary conditions for the magnetic field and the relativistic particle pressure in the jet, such as standard and advection-dominated accretion flow (ADAF) disc solutions. Surprisingly, the mass dependence of F-nu is very similar in different accretion scenarios. For typical flat-spectrum core-dominated radio jets and standard accretion scenarios, we find F-nu similar toM (17/12). The 7-9 orders of magnitude difference in black hole mass between microquasars and active galactic nuclei (AGN) jets imply that AGN jets must be about 3-4 orders of magnitude more radio-loud than microquasars, i.e. the ratio of radio to bolometric luminosity is much smaller in microquasars than in AGN jets. Because of the generality of these results, measurements of this F-nu-M dependence are a powerful probe of jet and accretion physics. We show how our analysis can be extended to derive a similar scaling relation between the accretion rate and F-nu for different accretion disc models. For radiatively inefficient accretion modes, we find that the flat-spectrum emission follows F-v proportional to (M(m) over dot)(17/12).
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