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  Dependence of the Gamma-Ray Emission from SN 1006 on the Astronomical Parameters

Ksenofontov, L., Berezhko, E., & Völk, H. (2005). Dependence of the Gamma-Ray Emission from SN 1006 on the Astronomical Parameters. In J. Blümer (Ed.), Contributions to the 29th International Cosmic Ray Conference (pp. 223-223). Karlsruhe: Forschungszentrum Karlsruhe.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-8A36-3 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-8A37-1
Genre: Conference Paper

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 Creators:
Ksenofontov, Leonid1, Author
Berezhko, Evgeni1, Author
Völk, Heinrich2, Author           
Affiliations:
1Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, 31 Lenin Ave., 677980 Yakutsk, Russia, ou_persistent22              
2Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907548              

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Free keywords: Supernova Remnants
 Abstract: We use nonlinear kinetic theory to study cosmic ray acceleration and the properties of the nonthermal emission from the supernova remnant SN 1006. The known range of astronomical parameters is examined in order to find out whether it encompasses the existing synchrotron emission data. It is shown that the hadronic gamma-ray flux is very sensitive to the ambient gas density NH and hat the existing H.E.S.S. upper limit requires NH < 0.1 cm-3. The amplified magnetic field downstream of the shock amounts to about 150 μG.

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Language(s): eng - English
 Dates: 2005
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 277790
URI: http://icrc2005.tifr.res.in/
 Degree: -

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Title: 29th International Cosmic Ray Conference
Place of Event: Pune, India
Start-/End Date: 2005-08-03 - 2005-08-10

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Title: Contributions to the 29th International Cosmic Ray Conference
Source Genre: Proceedings
 Creator(s):
Blümer, Johannes, Editor
Affiliations:
-
Publ. Info: Karlsruhe : Forschungszentrum Karlsruhe
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 223 - 223 Identifier: -