Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..253c&link_type=abstract
Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co
Astronomy and Astrophysics
Astrophysics
Scientific paper
The (candidates) black holes of our Galaxy live in couple with a star from which they accrete matter. These objects are commonly called X binary systems. These systems, persistent or transient, are very variable and a certain number of spectral states has been defined from the spectral and temporal properties observed in the X domain. This communication presents the X properties (caracteristic of the accretion) of these various spectral states. The recent development of the multi-wavelength observations (radio to hard X-ray) allows to better determine the physical phenomena involved in these spectral states. I present the recent results, obtained from the multi-wavelength analysis, allowing to better understand the accretion-ejection coupling around stellar black holes.
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