Unification of Spectral States of Accreting Black Holes

Details Unification of Spectral States of Accreting Black Holes Unification of Spectral States of Accreting Black Holes

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.355p&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a unifying radiation transfer model that can fit the spectral data in hard and soft states of Galactic black holes. We consider a hybrid thermal/non-thermal model where energy is injected to the hot corona by two channels: a non-thermal one (injection of energetic electrons), and a thermal one (that heats electrons). We show that the spectral transitions can be explained as a result of the redistribution of the energy dissipation between the cold disk and the hot corona (central hot accretion disc) with a constant non-thermal energy injection.

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