The electromagnetic emission from SCO X-1

Details The electromagnetic emission from SCO X-1 The electromagnetic emission from SCO X-1

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....55..111d&link_type=abstract

Astronomy and Astrophysics, vol. 55, no. 1, Feb. 1977, p. 111-116. Research supported by the Fundacao de Amparo a Pesquisa do E

Astronomy and Astrophysics

Astrophysics

2

Binary Stars, Electromagnetic Spectra, Emission Spectra, Neutron Stars, X Ray Sources, X Ray Stars, Atmospheric Heating, Stellar Atmospheres, Stellar Radiation, X Ray Spectra

Scientific paper

The spectrum of Sco X-1 in the range from 10 to the 14th power to 10 to the 20th power Hz is calculated, assuming that Sco X-1 is a binary system with a period of 0.787 days. The infrared and optical emission are produced in a hot spot of an X-ray-heated atmosphere of the primary star. The high-energy X-rays (above 40 keV) are emitted by the disk around the neutron star. The X-rays in the range 1-35 keV are emitted by the hot atmosphere of the neutron star, where the disk material is decelerated.

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