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Tidal disruption events (TDEs), in which stars are disrupted by supermassive black holes, have been proposed as potential sources of high-energy neutrinos through hadronic interactions. X-ray-bright TDEs provide dense photon fields…

High Energy Astrophysical Phenomena · Physics 2026-02-25 Rong-Lan Li , Chengchao Yuan , Hao-Ning He , Yun Wang , Ben-Yang Zhu , Yun-Feng Liang , Ning Jiang , Da-Ming Wei

The high-frequency radio sky is bursting with synchrotron transients from massive stellar explosions and accretion events, but the low-frequency radio sky has so far been quiet beyond the Galactic pulsar population and the long-term…

High Energy Astrophysical Phenomena · Physics 2025-03-12 N. Hurley-Walker , X. Zhang , A. Bahramian , S. J. McSweeney , T. N. O'Doherty , P. J. Hancock , J. S. Morgan , G. E. Anderson , G. H. Heald , T. J. Galvin

ASASSN-14ko is a periodically repeating nuclear transient. We conducted high-cadence, multiwavelength observations of this source, revealing several recurrent early bumps and rebrightenings in its UV/optical light curves. The energy…

MASTER OT 075353.88+174907.6 was a blue optical transient reported by the MASTER-Net project on 2017 Oct 31. This source was previously detected by {\it GALEX} in its NUV band but not by the Sloan Digital Sky Survey (in the optical). We…

High Energy Astrophysical Phenomena · Physics 2019-01-31 A. S. Parikh , J. V. Hernández Santisteban , R. Wijnands , D. Page

We present observations of the extremely luminous but ambiguous nuclear transient (ANT) ASASSN-17jz, spanning roughly 1200 days of the object's evolution. ASASSN-17jz was discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN)…

Fast Blue Optical Transients (FBOTs) are luminous transients with fast evolving (typically $t_{\rm rise}<12\ \rm days$) light curve and blue color (usually $\rm {-0.2\ >\ g-r\ >\ -0.3}$) that cannot be explained by a supernova-like…

High Energy Astrophysical Phenomena · Physics 2023-09-08 Chun Chen , Rong-Feng Shen

Some electromagnetic outbursts from the nuclei of distant galaxies have been found to repeat on months-to-years timescales, and each of these sources can putatively arise from the accretion flares generated through the repeated tidal…

High Energy Astrophysical Phenomena · Physics 2024-08-30 Ananya Bandopadhyay , Eric R. Coughlin , C. J. Nixon , Dheeraj R. Pasham

An examination of late-time, optical spectra of type Ia supernovae revealed surprisingly narrow absorption features which only become visible a few months after maximum light. These features, most clearly seen in the late-time spectra of…

High Energy Astrophysical Phenomena · Physics 2018-12-05 Christine S. Black , Robert A. Fesen , Jerod T. Parrent

Variations in stellar flux can potentially overwhelm the photometric signal of a transiting planet. Such variability has not previously been well-characterized in the ultraviolet lines used to probe the inflated atmospheres surrounding hot…

Solar and Stellar Astrophysics · Physics 2014-02-26 R. O. Parke Loyd , Kevin France

Galactic nuclei showing recurrent phases of activity and quiescence have recently been discovered, with recurrence times as short as a few hours to a day -- known as quasi-periodic X-ray eruption (QPE) sources -- to as long as hundreds to a…

We present a long-period radio transient (GLEAM-X J0704-37) discovered to have an optical counterpart, consistent with a cool main sequence star of spectral type M3. The radio pulsations occur at the longest period yet found, 2.9 hours, and…

[Abridged] We present a search for fast optical transients (~0.5 hr-1 day) using repeated observations of the Pan-STARRS1 Medium-Deep Survey (PS1/MDS) fields. Our search takes advantage of the consecutive g/r-band observations (16.5 min in…

Stars on bound orbits around a supermassive black hole may undergo repeated partial tidal disruption events (rpTDEs), producing periodic flares. While several candidates have been suggested, definitive confirmation of these events remains…

Recently an intriguing transient AT 2018lqh, with only a day-scale duration and a high luminosity of $7\times 10^{42}\ {\rm erg\ s^{-1}}$, has been discovered. While several possibilities are raised on its origin, the nature of this…

High Energy Astrophysical Phenomena · Physics 2021-12-08 Daichi Tsuna , Kazumi Kashiyama , Toshikazu Shigeyama

We present a detailed study of a transient in the center of SDSS1115+0544 based on the extensive UV, optical, mid-IR light curves (LC) and spectra over 1200 days. The host galaxy is a quiescent early type galaxy at $z$ = 0.0899 with a…

High Energy Astrophysical Phenomena · Physics 2019-03-27 Lin Yan , Tinggui Wang , Jiang Ning , Daniel Stern , Liming Dou , C. Fremling , M. J. Graham , A. J. Drake , Chenwei Yang , K. Burdge , M. M. Kasliwal

Three periastron passages of the PSR B1259$-$63/LS 2883 binary system, consisting of a 48 ms rotation-powered pulsar and a $\sim30$ M$_{\odot}$ Be star, have been observed by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space…

High Energy Astrophysical Phenomena · Physics 2018-08-15 T. J. Johnson , K. S. Wood , M. Kerr , R. H. D. Corbet , C. C. Cheung , P. S. Ray , N. Omodei

Wide-field survery have recently detected recurring optical and X-ray sources near galactic nuclei, with period spanning hours to years. These phenomena could result from repeated partial tidal disruptions of stars by supermassive black…

High Energy Astrophysical Phenomena · Physics 2023-11-10 Itai Linial , Eliot Quataert

Optical Transients from gamma-ray burst sources, in addition to offering a distance determination, convey important information on the physics of the emission mechanism, and perhaps also about the underlying energy source. As the gamma-ray…

Although flares from late-type main-sequence stars have been frequently detected in multi-wavelength, the associated dynamical process has been rarely reported so far. Here, we report follow-up observations of an X-ray transient triggered…

Solar and Stellar Astrophysics · Physics 2024-10-07 J. Wang , X. Mao , C. Gao , H. Y. Liu , H. L. Li , H. W. Pan , C. Wu , Y. Liu , G. W. Li , L. P. Xin , S. Jin , D. W. Xu , E. W. Liang , W. M. Yuan , J. Y. Wei

We investigate the flare-frequency distributions of 5 M-dwarfs that experienced superflares with energies in excess of $10^{33}$ erg detected by ASAS-SN. We use K2 and TESS short-cadence observations along with archival ASAS-SN data to…

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