Physical process which shapes Cassiopeia A
- 1 June 1987
- journal article
- research article
- Published by Springer Nature in Nature
- Vol. 327 (6121) , 395-398
- https://doi.org/10.1038/327395a0
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Secular changes within Cassiopeia A at 5 GHz-IMonthly Notices of the Royal Astronomical Society, 1986
- Jet with entrained clouds - I. Hydrodynamic simulations and magnetic field structureMonthly Notices of the Royal Astronomical Society, 1985
- Optical studies of Cassiopeia A. VII - Recent observations of the structure and evolution of the nebulosityThe Astrophysical Journal, 1985
- The Very Large ArrayThe Astrophysical Journal Supplement Series, 1980
- Proper motions and temporal flux changes of compact features in Cassiopeia A at 5 GHzMonthly Notices of the Royal Astronomical Society, 1977
- The Distribution of Linear Polarization in Cassiopeia A at Wavelengths of 9.8 and II. 1 CMThe Astronomical Journal, 1972
- Distribution of Brightness and Polarization in Cassiopeia A at 5.0 GHzMonthly Notices of the Royal Astronomical Society, 1970
- A New Intense Source of Radio-Frequency Radiation in the Constellation of CassiopeiaNature, 1948