Bacillus sp. X-3
National Institutes of Health
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The accretion disk around a compact object is a nonlinear general relativistic system involving magnetohydrodynamics. Naturally…
Some of the very high energy (VHE) gamma‐ray sources detected with the modern generation of Cherenkov telescopes have been…
We consider propagation of very high energy (VHE) gamma-rays in the radiation field of a massive star in the binary system Cen X…
COS-B viewed the Cyg X-3 region seven times between November, 1975, and February, 1982; a search for steady gamma-ray emission…
We have used the twin 11-m diameter mirrors of the NASA Jet Propulsion Laboratory's solar energy facility to observe high-energy…
According to the proposed model of the Cyg X-3, it should be recognized as a binary system consisting of a pulsar and an usual…
Observiations of γ rays of 1–20 MeV with the UCR Compton double scatter γ ray telescope are reported for a balloon flight…
THE detection of ∼ 100-MeV γ rays from Cyg X-3 has been reported from recently published SAS-2 data (R. C. Lamb et al.17). The…
CYGNUS X-3 has been identified1 with the infrared object found by Becklin et al.2 to be within ±2″ of the radio position: the…
CYGNUS X-3 is a candidate for the radio source which in September 1972 experienced a series of exceptional radio outbursts1. The…