Cold ultrarelativistic pulsar winds as potential sources of galactic gamma-ray 
lines above 100 GeV

Aharonian, F.A.; Khangulyan, D.; Malyshev, D.

doi:10.1051/0004-6361/201220092

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Cold ultrarelativistic pulsar winds as potential sources of galactic gamma-ray lines above 100 GeV

Aharonian, F., Khangulyan, D., & Malyshev, D. (2012). Cold ultrarelativistic pulsar winds as potential sources of galactic gamma-ray lines above 100 GeV. Astrophysics & Astronomy, 547: A114, pp. 1-6. doi:10.1051/0004-6361/201220092.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-000E-AD89-E Version Permalink: https://hdl.handle.net/11858/00-001M-0000-000E-AD8A-C

Genre: Journal Article

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Creators:
Aharonian, F.A.¹, Author
Khangulyan, D.¹, Author
Malyshev, D.², Author

Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550
2external, ou_persistent22

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Dates: Created: 2012-11Published Online: 2012-11-08

Publication Status: Published online

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Identifiers: DOI: 10.1051/0004-6361/201220092

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Title: Astrophysics & Astronomy

Other : Astrophys. Astron.

Source Genre: Journal

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Publ. Info: Berlin : Springer-Verlag

Pages: - Volume / Issue: 547 Sequence Number: A114 Start / End Page: 1 - 6 Identifier: ISSN: 0004-6361
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219