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Very High Resolution Calculations of Very Young Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

Eric M. Jones  and
Barham W. Smith
Eric M. Jones
Affiliation:
Los Alamos National Laboratory, University of California, Los Alamos, NM USA
Barham W. Smith
Affiliation:
Los Alamos National Laboratory, University of California, Los Alamos, NM USA

Extract

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After the supernova shock wave has swepted up about 8–10 stellar masses of interstellar material, the SNR structure is well described by blast wave theory (eg. Sedov 1959, Chevalier 1977). In fact, both numerical calculations of the early phases (Jones, Smith, and Straka 1981) and small scale, laboratory simulations (Wilke 1982) show transition to blast wave at 8–10 masses. While the late stages have been well understood for some time, the early stages have only been crudely modeled until very recently.

Type
I. Young Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 83 - 86
Copyright
Copyright © Reidel 1983 

References

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