SS Cygni as a hard X-ray source identified with the scanning modulation collimator on HEAO 1
- 1 October 1978
- journal article
- Published by Springer Nature in Nature
- Vol. 275 (5682) , 721-723
- https://doi.org/10.1038/275721a0
Abstract
No abstract availableThis publication has 5 references indexed in Scilit:
- Soft X-ray emission from Dwarf NovaeMonthly Notices of the Royal Astronomical Society, 1977
- The Structure of Cataclysmic VariablesAnnual Review of Astronomy and Astrophysics, 1976
- X-ray Emission from Accretion on to White DwarfsMonthly Notices of the Royal Astronomical Society, 1976
- Ultraviolet detection of the dwarf Nova SS Cyg.The Astrophysical Journal, 1974
- Possible Detection of Very Soft X-Rays from SS CygniThe Astrophysical Journal, 1974