On the periodical very high energy gamma-ray emission from Cyg X-3 |
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Authors: | Yu. I. Neshpor A. A. Stepanian V. P. Fomin S. A. Gerasimov B. M. Vladimirsky Yu. L. Ziskin |
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Affiliation: | (1) Crimean Astrophysical Observatory, Nauchny, Crimea, USSR |
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Abstract: | The period of very high energy (E>2×1012 eV) gamma-ray emission of Cyg X-3 by using the data of observations of the source made during 6 years, 1972–1977, was specified. The value of the period is equal to 0.199 683±1×10–6 days. Phase histogram reveals two peaks, one lagging the other by 0.6 of the period. The averaged 6 year data amounts to 1.8×10–10 quanta cm–2 s–1 (peak intensity). It corresponds to luminosity of about 1.2×1037 erg s–1 if one assumes that an emission is isotropical and the distance is equal to 10 kpc.
- E>2×1012 Cyg X-3 . 1972–1977 . - T=0,199 683 ±10–6 . , 0,6 . 1,8×10–10 –2 –1 ( ), 1,2×1037 / 10 . |
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