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  Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares

Kim, S.-H., Lee, S.-S., Lee, J. W., Hodgson, J. A., Kang, S., Algaba, J.-C., et al. (2022). Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares. \mnras, 510(1), 815-833. doi:10.1093/mnras/stab3473.

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 Creators:
Kim, Sang-Hyun, Author
Lee, Sang-Sung, Author
Lee, Jee Won, Author
Hodgson, Jeffrey A., Author
Kang, Sincheol, Author
Algaba, Juan-Carlos, Author
Kim, Jae-Young1, Author
Hodges, Mark, Author
Agudo, Ivan, Author
Fuentes, Antonio, Author
Escudero, Juan, Author
Myserlis, Ioannis1, Author
Traianou, Efthalia1, Author
Lähteenmäki, Anne, Author
Tornikoski, Merja, Author
Tammi, Joni, Author
Ramakrishnan, Venkatessh, Author
Järvelä, Emilia, Author
Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652              

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Free keywords: radiation mechanisms: non-thermal, galaxies: active, galaxies: jets, quasars: individual: CTA 102, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
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 Dates: 2022-02
 Publication Status: Issued
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 Identifiers: DOI: 10.1093/mnras/stab3473
BibTex Citekey: 2022MNRAS.510..815K
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Title: \mnras
Source Genre: Journal
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Pages: - Volume / Issue: 510 (1) Sequence Number: - Start / End Page: 815 - 833 Identifier: -