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What can the 2008/10 broadband flare of PKS 1502+106 tell us?. Nuclear opacity, magnetic fields, and the location of {γ} rays

MPS-Authors

Karamanavis,  V.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Fuhrmann,  L.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Angelakis,  E.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Nestoras,  I.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Myserlis,  I.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Krichbaum,  T.P.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Zensus,  J.A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Ungerechts,  H.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Sievers,  A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Gurwell,  M.A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Citation

Karamanavis, V., Fuhrmann, L., Angelakis, E., Nestoras, I., Myserlis, I., Krichbaum, T., et al. (2016). What can the 2008/10 broadband flare of PKS 1502+106 tell us? Nuclear opacity, magnetic fields, and the location of {γ} rays. Astronomy and Astrophysics, 590: A48, pp. A48. doi:10.1051/0004-6361/201527796.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002E-13ED-B
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