Emission lines from X ray binaries

Details Emission lines from X ray binaries Emission lines from X ray binaries

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..157k&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 157-161 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

4

Emission Spectra, K Lines, Ultraviolet Spectra, X Ray Binaries, X Ray Spectra, Accretion Disks, Spectral Signatures, Stellar Mass Accretion, Stellar Spectra

Scientific paper

Emission lines are probes of the conditions in the accretion flows associated with binary X-ray sources. The hard X-ray iron K line, soft X-ray lines, and UV lines, and what they indicate about the conditions in binary X-ray sources are discussed. These lines are interpreted using an X-ray illuminated accretion disk model. The structure and dynamics of the heated disk, its spectral signatures, and the major unsolved theoretical issues surrounding them are investigated.

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