Absorption anomalies in compact X-ray sources

Details Absorption anomalies in compact X-ray sources Absorption anomalies in compact X-ray sources

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apl....16..121g&link_type=abstract

Astrophysical Letters, vol. 16, no. 3, 1975, p. 121-123.

Astronomy and Astrophysics

Astrophysics

7

Absorption Spectra, Interstellar Extinction, Stellar Spectra, X Ray Sources, Anomalies, Binary Stars, Emission Spectra, Error Analysis, Hydrogen, X Ray Spectra

Scientific paper

It is suggested that the apparently deficient interstellar X-ray
absorption along the line of sight to compact X-ray sources must be due
to a soft X-ray emission excess. Suitable multiple-emission regions are
predicted to exist in accretion disks. Examples of this feature are
found in Cyg X-1 and Sco X-1.

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