Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980nyasa.336..550m&link_type=abstract
In: Texas Symposium on Relativistic Astrophysics, 9th, Munich, West Germany, December 14-19, 1978, Proceedings. (A80-42502 18-90
Astronomy and Astrophysics
Astrophysics
14
Galactic Radiation, Light Emission, Stellar Spectra, Stellar Spectrophotometry, X Ray Sources, Balmer Series, H Alpha Line, Heao 2, Infrared Spectra, Pulsars, Satellite-Borne Instruments, Stellar Atmospheres, Stellar Luminosity
Scientific paper
Optical counterparts of compact galactic X-ray sources are discussed, with emphasis on sources with X-ray luminosities in the 10 to the 36th to 10 to the 38th erg/s range within the bandpass 1-10 keV. Also considered is recent progress on optical identifications of galactic X-ray sources with luminous (M(V) less than O) visible counterparts, as well as progress in the fast photometry of the counterparts of X-ray pulsars. In addition, counterparts of Scorpius X-1-like sources and of X-ray bursters are examined along with Balmer line profiles and the red/infrared spectrum of SS 433.
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