The pertinence of jet emitting discs in microquasars theory and comparison to observations

Details The pertinence of jet emitting discs in microquasars theory and comparison to observations The pertinence of jet emitting discs in microquasars theory and comparison to observations

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010sf2a.conf..195p&link_type=abstract

SF2A-2010: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: S. Boissier, M. Heydari-

Astronomy and Astrophysics

Astrophysics

X-Rays: Binaries, Accretion, Accretion Disks, Magnetic Fields: Mhd

Scientific paper

Jet Emitting Disc (JED) has dynamical properties quite different from both the standard and advection dominated discs. It also exhibits three different thermal equilibrium branches at a given radius: two stable (cold and hot) and one intermediate unstable. The hot solution has all the characteristics of the so-called "hot corona" generally invoked in XrB sytems in the Low/Hard states. We detail the energetics and radiative expectations of our model and show their good agreement with those observed in Cygnus X-1 in terms of jet power, jet velocity and spectral emission.

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