An Evaluation of the Richtmyer‐Meshkov Instability in Supernova Remnant Formation
Open Access
- 20 January 1999
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 511 (1) , 335-340
Abstract
No abstract availableKeywords
This publication has 39 references indexed in Scilit:
- X-Ray and Ultraviolet Line Emission from SNR 1987AThe Astrophysical Journal, 1997
- Axisymmetric Circumstellar Interaction in SupernovaeThe Astrophysical Journal, 1996
- Power Laws and Similarity of Rayleigh-Taylor and Richtmyer-Meshkov Mixing Fronts at All Density RatiosPhysical Review Letters, 1995
- On the X-ray spectrum of Kepler's supernova remnantThe Astrophysical Journal, 1994
- Scale invariant mixing rates of hydrodynamically unstable interfacesPhysical Review Letters, 1994
- Dynamics of Kepler's supernova remnantThe Astrophysical Journal, 1992
- Hydrodynamic instabilities in supernova remnants - Self-similar driven wavesThe Astrophysical Journal, 1992
- The origin of Kepler's supernova remnantThe Astrophysical Journal, 1987
- Self-similar solutions for the interaction of stellar ejecta with an external mediumThe Astrophysical Journal, 1982
- Early Supernova LuminosityThe Astrophysical Journal, 1969