Two-component continuum spectrum in X-ray pulsar EXO2030+375

Details Two-component continuum spectrum in X-ray pulsar EXO2030+375 Two-component continuum spectrum in X-ray pulsar EXO2030+375

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..383s&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 13, no. 12, p. (12)383-(12)386

Astronomy and Astrophysics

Astronomy

Black Body Radiation, Curve Fitting, Pulsars, Stellar Models, Stellar Temperature, X Ray Astronomy, X Ray Spectra, B Stars, Computer Programs, Error Analysis, Exosat Satellite, Gamma Ray Observatory, Ginga Satellite

Scientific paper

We report the detection of a soft X-ray component in the spectrum of the
transient X-ray pulsar EXO2030+375 at a high state in 1985. The spectrum
of the soft X-ray component could be fitted by a blackbody with a
temperature kT approx. 1.1 keV and a radius of the emission area R
approx. 3.6 - 6.1 km (assuming 5 kpc distance).

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