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  A method for computing synchrotron and inverse-Compton emission from hydrodynamic simulations of supernova remnants

Obergaulinger, M., Chimeno, J., Mimica, P., Aloy, M., & Iyudin, A. (2015). A method for computing synchrotron and inverse-Compton emission from hydrodynamic simulations of supernova remnants. High Energy Density Physics, 17, Part A Special Issue, 92-97.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0029-57E9-7 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0029-57EA-5
Genre: Conference Paper

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 Creators:
Obergaulinger, M., Author
Chimeno, J.M., Author
Mimica, P., Author
Aloy, M.Á., Author
Iyudin, A.1, Author              
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2015-12
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Method: Peer
 Identifiers: DOI: 10.1016/j.hedp.2014.11.004
Other: LOCALID: 2242041
 Degree: -

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Title: 10th International Conference on High Energy Density Laboratory Astrophysics
Place of Event: Bordeaux, France
Start-/End Date: 2014-05-12 - 2014-05-16

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Title: High Energy Density Physics
  Abbreviation : High Energy Density Phys.
Source Genre: Journal
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Publ. Info: -
Pages: 6 Volume / Issue: 17, Part A Special Issue Sequence Number: - Start / End Page: 92 - 97 Identifier: ISSN: 1574-1818
ISSN: 1878-0563