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- W3146504544 abstract "The emission mechanism from X-ray soturces in close binary stars is studied.It is suggested that pair production may play an important role in the X-ray emission region which is formed by the accretion of a compact object(a neutron star or a black hole).The present model accounts qualitatively for the following observed general properties in X-ray binaries: 1.The X-ray luminosity lies within the range 10~(36)—10~(38)erg/sec. 2.The X-ray energy spectrum can in the majority of cases be represented either the power-law or the thermal bremsstrahlung form. 3.The temperature of the thermal bremsstrahlung spectrum is the order of 10~8K. 4.The form of the energy spectrum does not change appreciably when the luminosity fluctuates." @default.
- W3146504544 created "2021-04-13" @default.
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- W3146504544 date "1975-01-01" @default.
- W3146504544 modified "2023-09-28" @default.
- W3146504544 title "AN INTERPRATATION OF THE GENERAL CHARACTER OF THE X-RAY EMISSION FROM COMPACT OBJECTS IN CLOSE BINARY STARS" @default.
- W3146504544 hasPublicationYear "1975" @default.
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