BRITZEN, S., C. FENDT, A. TRAMACERE, I. N. PASHCHENKO, F. JARON, Radim PÁNIS, L. PETROV, M. F. ALLER, H. D. ALLER, Michal ZAJACEK and L. C. POPOVIC. A ring accelerator? Unusual jet dynamics in the IceCube candidate PKS 1502+106. Monthly Notices of the Royal Astronomical Society. GB - Spojené království Velké Británie a, 2021, vol. 503, No 3, p. 3145-3178. ISSN 0035-8711. Available from: https://dx.doi.org/10.1093/mnras/stab589.
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Basic information
Original name A ring accelerator? Unusual jet dynamics in the IceCube candidate PKS 1502+106
Authors BRITZEN, S., C. FENDT, A. TRAMACERE, I. N. PASHCHENKO, F. JARON, Radim PÁNIS (703 Slovakia, belonging to the institution), L. PETROV, M. F. ALLER, H. D. ALLER, Michal ZAJACEK and L. C. POPOVIC.
Edition Monthly Notices of the Royal Astronomical Society, GB - Spojené království Velké Británie a, 2021, 0035-8711.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/21:A0000140
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1093/mnras/stab589
UT WoS 000649000600003
Keywords in English astroparticle physics;black hole physics;techniques: interferometric;galaxies: active;galaxies: jets;quasars: individual: PKS 1502+106
Tags 2022, EF19-073 0016951, , RIV22, SGF-4-2020, SGS-12-2019
Tags International impact, Reviewed
Links EF19_073/0016951, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 28/3/2022 08:19.
Abstract
On 2019/07/30.86853 UT, IceCube detected a high-energy astrophysical neutrino candidate. The Flat Spectrum Radio Quasar PKS 1502+106 is located within the 50 per cent uncertainty region of the event. Our analysis of 15 GHz Very Long Baseline Array (VLBA) and astrometric 8 GHz VLBA data, in a time span prior and after the IceCube event, reveals evidence for a radio ring structure that develops with time. Several arc-structures evolve perpendicular to the jet ridge line. We find evidence for precession of a curved jet based on kinematic modelling and a periodicity analysis. An outflowing broad line region (BLR) based on the C IV line emission (Sloan Digital Sky Survey) is found. We attribute the atypical ring to an interaction of the precessing jet with the outflowing material. We discuss our findings in the context of a spine-sheath scenario where the ring reveals the sheath and its interaction with the surroundings (narrow line region, NLR, clouds). We find that the radio emission is correlated with the gamma-ray emission, with radio lagging the gamma-rays. Based on the gamma-ray variability time-scale, we constrain the gamma-ray emission zone to the BLR (30-200 r(g)) and within the jet launching region. We discuss that the outflowing BLR provides the external radiation field for gamma-ray production via external Compton scattering. The neutrino is most likely produced by proton-proton interaction in the blazar zone (beyond the BLR), enabled by episodic encounters of the jet with dense clouds, i.e. some molecular cloud in the NLR.
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