The detection of the hard component in the radiation spectrum of the X-ray nova in Vulpecula - Preliminary results from the KVANT module

Details The detection of the hard component in the radiation spectrum of the X-ray nova in Vulpecula - Preliminary results from the KVANT module The detection of the hard component in the radiation spectrum of the X-ray nova in Vulpecula - Preliminary results from the KVANT module

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..771s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Sept. 1988, p. 771-786. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

8

Astronomical Spectroscopy, Novae, Radiation Spectra, X Ray Sources, Black Holes (Astronomy), Compton Effect, Cosmic Plasma, Light Curve

Scientific paper

Two components were detected in the spectrum of the X-ray nova in
Vulpecula. A soft component is found to be dominant in the 4-15 keV
band. A hard power law component accounts for 10 percent of the source
luminosity and dominates the spectrum in the 15-200 keV band. An energy
drop is observed above 200 keV.

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