Observations of CYG X-1 from Aryabhata

Astronomy and Astrophysics – Astronomy

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Spaceborne Astronomy, Stellar Spectrophotometry, X Ray Stars, Indian Space Program, Photon Density, Proportional Counters, Satellite-Borne Instruments, Stellar Spectra, X Ray Astronomy

Scientific paper

The paper reports results of observations of the X-ray source Cyg X-1 by the Indian satellite Aryabhata on April 19, 1975. The observations of the source were made by proportional counter telescopes in the energy range 2.5 to 18.75 keV just before the source made a major increase in its intensity. The spectrum of Cyg X-1 thus detected shows a power law dependence with an index of about 0.7 plus or minus 0.2 in the energy interval 2.5-13.8 keV, the estimated intensity being 0.84 plus or minus 0.3 photons/sq. cm/s. The source underwent a major upward transition in its intensity during late April. This intensity transition is characterized by an accompanying spectral change with spectral exponent changing from the value of 1.6 during the normal state to 2.2 in the 'high' state.

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