Astronomy and Astrophysics – Astronomy
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..297k&link_type=abstract
In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 297-299 (SEE N94-22624 05-75)
Astronomy and Astrophysics
Astronomy
2
Black Holes (Astronomy), Novae, Stellar Radiation, X Ray Spectra, Compton Effect, Emission Spectra, Light (Visible Radiation), Plasma Jets, X Ray Stars
Scientific paper
Some properties of x ray novae, considered to contain a black hole are described. 71% of the black hole candidates belong to x ray novae. From the spectral study of these novae, at the rising phase, the appearance of hard x rays beyond 100 keV is found. The origin of these hard x rays is described. The probability that a black hole candidate is an x ray nova is shown. The observation of a component comptonized by hot electrons around the soft x ray peak indicates the existence of nonthermal energetic phenomena at the early phase of the nova activity. A model including jet phenomena is discussed.
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