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The Effect of Dust Sputtering in Supernova Remnant

Published online by Cambridge University Press:  25 May 2016

Takashi Kurino ,
Masayuki Fujimoto  and
Asao Habe
Takashi Kurino
Affiliation:
Astrophysics Labolatory Division of Physics, Graduate School of Science, HOKKAIDO University Kita 10 Nishi 8, Sapporo, Hokkaido 060, JAPAN
Masayuki Fujimoto
Affiliation:
Astrophysics Labolatory Division of Physics, Graduate School of Science, HOKKAIDO University Kita 10 Nishi 8, Sapporo, Hokkaido 060, JAPAN
Asao Habe
Affiliation:
Astrophysics Labolatory Division of Physics, Graduate School of Science, HOKKAIDO University Kita 10 Nishi 8, Sapporo, Hokkaido 060, JAPAN

Extract

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IRAS observations of supernova remnants (SNRs) reported that infrared luminosity from SNRs are very different, though some of them have same temperature. This is because infrared emittion depends on density of the dust grains.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 253
Copyright
Copyright © Kluwer 1998 

References

Dwek, Eli The Infrared Diagnostic of a Dusty Plasma with Applications to Supernova Remnantos. Apj, 322, 812–821 CrossRefGoogle Scholar
Draine, B. T. and Woods, D.T. Supernova Remnants in Dense Clouds, I, Blast-Wave Dynamics and X-ray Irradiation. Apj, 383, 621–638 CrossRefGoogle Scholar