Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..42..175p&link_type=abstract
(COSPAR, Symposium on Fast Transients in X- and Gamma-Rays, Varna, Bulgaria, May 29-31, 1975.) Astrophysics and Space Science, v
Astronomy and Astrophysics
Astronomy
13
Astronomical Netherlands Satellite, Binary Stars, Spaceborne Astronomy, Stellar Luminosity, Stellar Spectra, X Ray Stars, Astronomical Spectroscopy, Light Curve, Photon Density, Radiant Flux Density, Radiation Detectors, Satellite Observation, Spectral Energy Distribution, X Ray Astronomy, X Ray Spectra
Scientific paper
Cygnus X-1 was observed from 3 November until 9 November 1974, using the hard X-ray (1-28 keV) and soft X-ray (1-8 keV) experiment on board the Astronomical Netherlands Satellite. On three occasions, on 4 and 5 November, the X-ray spectrum was observed to be harder, while the flux intensity in the 1-7 keV ranges decreased by about 50% from its quiescent value. These events occurred near and following the time of superior conjunction of the likely optical counterpart HDE 226 868. These events appear to be the same as previously reported absorption dips and reveal this phenomenon to be more complex than had been believed. A systematic study of the X-ray spectral variations in these energy bands, on a time scale of 64 seconds over the period of the spectroscopic binary, is presented.
Brinkman Albert C.
Epstein Adam
Grindlay Jonathan
Gursky Herbert
Heise Jaret
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