Broadband X-ray spectra of black hole candidates, X-ray pulsars, and low-mass X-ray binaries - Results from the KVANT module

Details Broadband X-ray spectra of black hole candidates, X-ray pulsars, and low-mass X-ray binaries - Results from the KVANT module Broadband X-ray spectra of black hole candidates, X-ray pulsars, and low-mass X-ray binaries - Results from the KVANT module

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..975s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Nov. 1991, p. 975-984. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

5

Black Holes (Astronomy), Neutron Stars, Stellar Spectra, X Ray Binaries, X Ray Spectra, Mir Space Station, Pulsars, Stellar Magnetic Fields

Scientific paper

The broadband spectra of the brightest X-ray sources observed by the TTM, Hexe, and Pulsar X-1 devices of the Kvant module are discussed. They demonstrate the differences in the hardness of the spectra of neutron stars with a weak magnetic field, namely, Sco X-1, X-ray pulsars A0535 + 26, Vela X - 1, LMC X - 4, and the black hole candidates Cyg X - 1, GS2023 + 338, GS2000 + 25, and 3C273.

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