Ultraviolet spectroscopy of the X-ray binary HZ Her/Her X-1

Details Ultraviolet spectroscopy of the X-ray binary HZ Her/Her X-1 Ultraviolet spectroscopy of the X-ray binary HZ Her/Her X-1

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.263..471b&link_type=abstract

In ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE p 471-47

Astronomy and Astrophysics

Astrophysics

8

Line Spectra, Stellar Spectra, Ultraviolet Spectroscopy, X Ray Binaries, Center Of Gravity, Iue, Spatial Distribution, Stellar Models, Stellar Spectrophotometry

Scientific paper

High and low resolution spectra of HZ Her are being examined to probe the primary site of line emission. The N V emission lines show a very small range of velocities; they must be formed in the X-ray "heated" hemisphere of the mass donor, within which lies the barycentre of the system. Line fluxes from low resolution spectrophotometry are being compared with simple models to investigate the spatial distribution of the line forming regions.

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