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RAS PhysicsАстрономический журнал Astronomy Reports

  • ISSN (Print) 0004-6299
  • ISSN (Online) 3034-5170

INFRARED AND X-RAY EMISSION OF A SUPERNOVA REMNANT IN A CLUMPY MEDIUM

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PII
S30345170S0004629925030016-1
DOI
10.7868/S3034517025030016
Publication type
Article
Status
Published
Authors
S. Yu. Dedikov
  • Affiliation: P. N. Lebedev Physical Institute of the Russian Academy of Sciences
E. O. Vasiliev
  • Affiliation: P. N. Lebedev Physical Institute of the Russian Academy of Sciences
Volume/ Edition
Volume 102 / Issue number 3
Pages
159-169
Abstract
The infrared (IR) to X-ray luminosity ratio (IRX) is an indicator of the role of the dust plays in cooling of hot gas in supernova remnants (SNR). Using the 3D dynamics of gas and interstellar polydisperse dust grains we analyzed the evolution of SNR in the inhomogeneous medium. We obtained spatial distributions of the surface brightness both of the X-ray emission from hot gas inside SNR and the IR emission from the SNR swept-up shell, as well as, the average gas temperature in the SNR,
Keywords
галактики межзвездная среда оболочки ударные волны остатки сверхновых пыль
Date of publication
11.11.2024
Year of publication
2024
Number of purchasers
0
Views
43

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