| Issue |
A&A
Volume 390, Number 3, August II 2002
|
|
|---|---|---|
| Page(s) | 1063 - 1074 | |
| Section | The Sun | |
| DOI | https://doi.org/10.1051/0004-6361:20020731 | |
| Published online | 14 August 2002 | |
The evolution of mass loaded supernova remnants
I. Constant and Mach Number dependent mass injection rates
1
Department of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT, UK
2
Instituto de Astronomia, UNAM, Campus Morelia, Apartado Postal 3-72, 58090 Morelia, Michoacán, Mexico
Corresponding author: S. J. Arthur, j.arthur@astrosmo.unam.mx
Received:
8
February
2002
Accepted:
15
May
2002
We describe the evolution of spherically symmetric supernova remnants in which mass addition takes place from embedded clouds. We derive simple approximations to the remnant evolution which can be used for investigating the generation of supernova induced phenomena such as galactic superwinds.
Key words: ISM: kinematics and dynamics / ISM: supernova remnants / galaxies: ISM
© ESO, 2002
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