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

Obergaulinger, M.; Chimeno, J.M.; Mimica, P.; Aloy, M.Á.; Iyudin, A.

doi:10.1016/j.hedp.2014.11.004

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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: https://hdl.handle.net/11858/00-001M-0000-0029-57E9-7 Version Permalink: https://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: Date issued: 2015-12

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1016/j.hedp.2014.11.004
Other: LOCALID: 2242041

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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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Pages: 6 Volume / Issue: 17, Part A Special Issue Sequence Number: - Start / End Page: 92 - 97 Identifier: ISSN: 1574-1818
ISSN: 1878-0563