Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006
Open Access
- 1 November 1995
- journal article
- letter
- Published by Springer Science and Business Media LLC in Nature
- Vol. 378 (6554), 255-258
- https://doi.org/10.1038/378255a0
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- HEAO 1 A-2 low-energy detector X-ray spectra of the Lupus Loop and SN 1006The Astrophysical Journal, 1991
- Self-consistent models for the X-ray emission from supernova remnants - an application to Kepler's remnantThe Astrophysical Journal, 1985
- Imaging X-ray spectrophotometric observation of SN 1006The Astrophysical Journal, 1985
- X-ray line emission from supernova remnants. I - Models for adiabatic remnantsThe Astrophysical Journal Supplement Series, 1983
- An X-ray map of SN 1006 from the Einstein ObservatoryMonthly Notices of the Royal Astronomical Society, 1981
- Is the remnant of SN 1006 CrablikeThe Astrophysical Journal, 1980
- X-ray spectrum of Kepler's supernova remnantThe Astrophysical Journal, 1980
- Elemental abundances in a Type I supernova remnantThe Astrophysical Journal, 1980
- X-ray spectrum of Cassiopeia A measured with the Einstein SSSThe Astrophysical Journal, 1979
- The supernova of AD 1006Monthly Notices of the Royal Astronomical Society, 1977