Galactic microquasars and "canonical" states of black-hole candidates

Details Galactic microquasars and "canonical" states of black-hole candidates Galactic microquasars and "canonical" states of black-hole candidates

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.325b&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

The X-ray properties of the only two known superluminal galactic sources are extremely complex and different from those of `conventional' black-hole candidates. Nevertheless, many characteristics of GRS 1915+105 and GRO J1655-40 are not unlike those expected from black-hole candidates on the basis of other known sources. I examine the timing and spectral properties of these two sources in terms of canonical black-hole states, concentrating on the similarities rather than on the peculiarities.

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