Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-07T19:46:34.424Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  24 February 2011

Pierre-Olivier Petrucci
Affiliation:
Laboratoire d'Astrophysique de GrenOble, Université Joseph Fourier - Grenoble 1 / CNRS UMR 5571, BP 53, 38041 Grenoble Cedex 09, France email: [email protected]
Jonathan Ferreira
Affiliation:
Laboratoire d'Astrophysique de GrenOble, Université Joseph Fourier - Grenoble 1 / CNRS UMR 5571, BP 53, 38041 Grenoble Cedex 09, France email: [email protected]
Gilles Henri
Affiliation:
Laboratoire d'Astrophysique de GrenOble, Université Joseph Fourier - Grenoble 1 / CNRS UMR 5571, BP 53, 38041 Grenoble Cedex 09, France email: [email protected]
Julien Malzac
Affiliation:
Centre d'Etude Spatial des Rayonnement UMR 5187 9, av du Colonel Roche BP 44346 31028 Toulouse Cedex 4France
Cedric Foellmi
Affiliation:
Laboratoire d'Astrophysique de GrenOble, Université Joseph Fourier - Grenoble 1 / CNRS UMR 5571, BP 53, 38041 Grenoble Cedex 09, France email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Blandford, R. D. & Payne, D. G. 1982, MNRAS, 199, 883CrossRefGoogle Scholar
Ferreira, J. & Pelletier, G. 1993, A&A, 276, 625+Google Scholar
Malzac, J., Belmont, R., & Fabian, A. C. 2009, MNRAS, 400, 1512CrossRefGoogle Scholar
Petrucci, P.-O., Ferreira, J., Henri, G., Malzac, J., & Foellmi, C. 2010, A&A, in press (arXiv:1007.1478)Google Scholar