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2026 年 6 月 20 日 星期六 · 数据截至 arXiv / ADS 最新收录日
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优先级 80 · 多信使触发与联合 · 高能暂现天体

Multiwavelength variability of the high-energy neutrino candidate PKS 0735+178 over three decades

高能中微子候选体 PKS 0735+178 三十年的多波段光变

T. V. Mufakharov (State Key Laboratory of Radio Astronomy and Technology, Xinjiang Astronomical Observatory, CAS; Special Astrophysical Observatory of the Russian Academy of Sciences), Yu. V. Sotnikova (Special Astrophysical Observatory of the Russian Academy of Sciences; Institute for Nuclear Research, Russian Academy of Sciences), V. V. Vlasyuk (Special Astrophysical Observatory of the Russian Academy of Sciences) et al.

原文摘要Abstract

We present the multiwavelength variability of the BL Lac object PKS 0735+178, associated with the high-energy neutrino event IC211208A. The light curves cover the radio (1─230 GHz), optical, and Fermi-LAT <inline-formula><tex-math>$\gamma$</tex-math></inline-formula>-ray bands over a <inline-formula><tex-math>$\sim$</tex-math></inline-formula>30 yr time-scale. The light curves are correlated, with delays from 0 to 1200 d increasing towards lower frequencies, consistent with emission from an opacity-stratified jet. The bright flare after the IC211208A event indicates emission from a compact, optically thick region with enhanced activity and more efficient particle acceleration. Short optical and <inline-formula><tex-math>$\gamma$</tex-math></inline-formula>-ray bursts have been detected very close to the neutrino event, within a few days. The <inline-formula><tex-math>$\sim$</tex-math></inline-formula>12-d lag between the <inline-formula><tex-math>$\gamma$</tex-math></inline-formula>-ray and optical emissions is detected for the first time, suggesting that the emission regions are not co-spatial. A characteristic variability time-scale of <inline-formula><tex-math>$\sim$</tex-math></inline-formula>10─11 yr is robustly detected in the radio─mm bands (<inline-formula><tex-math>${\ge} 3\sigma$</tex-math></inline-formula>), while the optical and <inline-formula><tex-math>$\gamma$</tex-math></inline-formula>-ray data show weaker, shorter period signals. The independent constraints from the VLBI core-shift measurements and radio time delays yield consistent estimates of the jet geometry and disturbance propagation, supporting variability governed by jet propagation effects. The long-term modulation is consistent with a slow variation in energy release at the jet base, while individual flares arise from shocks propagating downstream. Jet precession may contribute to the long-term modulation; however, the required viewing angles are inconsistent with the VLBI constraints, indicating that precession alone cannot explain the observed variability.

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亮点

首次可靠测定PKS 0735+178伽马射线与光学波段间约12天延迟,表明辐射区非共空间;在射电至毫米波段稳健探测到~10–11年准周期光变,并结合VLBI核位移测量对喷流几何和扰动传播给出自洽约束。

脉络与展望

PKS 0735+178作为高能中微子事件IC211208A的可能对应体(IceCube Collaboration 2021Acharyya+ 2023),先前已被发现具有长期光变和准周期行为(Fan+ 1997Qian and Tao 2004Ciprini+ 2007)。VLBI观测揭示其喷流视角很小、存在弯曲和超光速运动(Weaver+ 2022Agudo+ 2006)。本研究通过约30年的多波段数据,将频率依赖的时间延迟与VLBI核位移测量相结合,支持了激波在分层喷流中传播的图像(如Konigl 1981Lobanov 1998所描述的模型框架)。未来更高时间分辨率和更多中微子候选体的联合监测,有望进一步区分喷流几何进动(例如Britzen+ 2023讨论的进动模型)与内禀能量释放调制对长期光变的贡献,并检验多区域辐射机制。

预印本 2026-06-20 · 刊出 2026-06-22 · 收录 2026-07-22