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Is there a non-stationary γ-ray emission zone 42 pc from the 3C 279 core?

Patiño-Álvarez, V., Dzib, S., Lobanov, A., & Chavushyan, V. (2019). Is there a non-stationary γ-ray emission zone 42 pc from the 3C 279 core? aap, 630: A56, pp. A56. doi:10.1051/0004-6361/201834401.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0006-78A0-E Version Permalink: https://hdl.handle.net/21.11116/0000-0006-78A1-D

Genre: Journal Article

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Patiño-Álvarez, V.M.¹, Author
Dzib, S.A.¹, Author
Lobanov, A.¹, Author
Chavushyan, V., Author

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1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652

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Free keywords: \ensuremath{γ} rays: galaxies, radiation mechanisms: non-thermal, quasars: individual: 3C 279, galaxies: active, techniques: high angular resolution, Astrophysics - High Energy Astrophysical Phenomena

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Dates: Date issued: 2019-10

Publication Status: Issued

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Identifiers: DOI: 10.1051/0004-6361/201834401
BibTex Citekey: 2019A&A...630A..56P

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Title: aap

Source Genre: Journal

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Pages: - Volume / Issue: 630 Sequence Number: A56 Start / End Page: A56 Identifier: -