The X ray spectrum of Nova VUL 1988. Mir-Kvant data

Details The X ray spectrum of Nova VUL 1988. Mir-Kvant data The X ray spectrum of Nova VUL 1988. Mir-Kvant data

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296...15e&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 15-17 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

1

Mir Space Station, Novae, Stellar Spectra, X Ray Spectra, Data Acquisition, Stellar Mass Accretion, X Ray Astronomy, X Ray Binaries

Scientific paper

The X-ray spectrum of the two components, detected in Vulpeca GS
2000+25, are presented. Two components of X-ray spectrum were detected:
a soft component with a temperature of 20 million Kelvin and a hard
component up to the energy 200 to 300 keV. Soft component dominates in
the 4 to 15 keV band and contains 90 percent of the source luminosity.

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