Accueil > Séminaires d’Astrophysique > The evolution of black hole binaries

 

The evolution of black hole binaries

Tomaso Belloni (INAF - Osservatorio Astronomico di Brera, Merate, Italie)

Par Stephane Charpinet - 28/09/2007

 

Séminaires d’Astrophysique

de l’Observatoire Midi-Pyrénées


Séminaire de

Tomaso BELLONI

 (INAF - Osservatorio Astronomico di Brera, Merate, Italie)

Jeudi 8 Novembre 2007 à 11h

CESR


The evolution of black hole binaries

The past decade has seen an incredible increase in the amount of available X-ray data of black-hole binaries, thanks to the RossiXTE satellite. At the same time, the development of solid multi- wavelength programs has led to the discovery of relativistic jets from these systems and their complex relation to the accretion properties. Although the phenomenology appears at first sight to be intractable, delving into the trove of available data and using appropriate tools, it is possible to reach basic conclusions about the spectral/timing behaviour during the outburst of transient systems. I will describe the unified picture that we have reached for transient systems and how it can be connected to the properties of jet ejection. This paradigm can be applied also to persistent systems such as Cygnus X-1 and even to Active Galactic Nuclei.

 

 

[Page Précédente] [Dans la même rubrique] [Sommaire]

 

 

Site du CNRS Logo OMP
Logo UPS
Logo INSU-CNRS

Annuaire

Rechercher

Sur ce site



Bibliotheque

Laboratoire Astrophysique de Toulouse - Tarbes (UMR5572)

CNRS (Midi-Pyrénées)

Univ. Paul Sabatier

Liens utiles

Accueil Imprimer Contact mail Plan du site Crédits