Coincidence of compact supernova remnants with three COS-B γ-ray sources
- 1 March 1978
- journal article
- Published by Springer Nature in Nature
- Vol. 272 (5652) , 429-430
- https://doi.org/10.1038/272429a0
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- New high energy γ-ray sources observed by COS BNature, 1977
- The Interaction of Supernovae with the Interstellar MediumAnnual Review of Astronomy and Astrophysics, 1977
- Final SAS-2 gamma-ray results on sources in the galactic anticenter regionThe Astrophysical Journal, 1977
- Observation of gamma rays with a 4.8 hour periodicity from Cygnus X-3The Astrophysical Journal, 1977
- A Study of Galactic Supernova Remnants, Based on Molonglo–Parkes Observational DataMonthly Notices of the Royal Astronomical Society, 1976
- SAS-2 high-energy gamma-ray observations of the VELA pulsarThe Astrophysical Journal, 1975
- Gamma radiation from the Crab Nebula above 35 MeVNature, 1974
- Polarization of supernova remnants KE 69, G 357.7-0.1, HC 26, and gamma Cygni at 6- and 2.8-cm wavelengths.The Astronomical Journal, 1974
- Pulsars and the Distribution of Celestial Gamma RaysPhysical Review Letters, 1970
- Supernova Remnants as Radio SourcesAustralian Journal of Physics, 1968