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Recent UV-optical surveys have been successful in finding tidal disruption events (TDEs), in which a star is tidally disrupted by a supermassive black hole (BH). These TDEs release a huge amount of radiation energy ~ 10^51-52 erg into the…

High Energy Astrophysical Phenomena · Physics 2016-02-17 Wenbin Lu , Pawan Kumar , Neal J. Evans

We present predictions for time delays between multiple images of the gravitationally lensed supernova, iPTF16geu, which was recently discovered from the intermediate Palomar Transient Factory (iPTF). As the supernova is of Type Ia where…

Cosmology and Nongalactic Astrophysics · Physics 2017-02-08 Anupreeta More , Sherry H. Suyu , Masamune Oguri , Surhud More , Chien-Hsiu Lee

Tidal disruption events which repeat on timescales of months-to-years represent an unambiguous signature of a partial disruption, with the surviving stellar remnant returning to pericentre to be repeatedly stripped by tidal forces. These…

High Energy Astrophysical Phenomena · Physics 2026-02-24 Andrew Mummery

(abridged) The heating mechanism at high densities during M dwarf flares is poorly understood. Spectra of M dwarf flares in the optical and near-ultraviolet wavelength regimes have revealed three continuum components during the impulsive…

Solar and Stellar Astrophysics · Physics 2015-06-23 Adam F. Kowalski , Suzanne L. Hawley , Mats Carlsson , Joel C. Allred , Han Uitenbroek , Rachel A. Osten , Gordon Holman

We report on the variability of a multi-component broad absorption line (BAL) system observed in the hyper-luminous quasar J1538+0855 at z=3.6. Observations from SDSS, VLT, LBT and Subaru telescopes taken at five different epochs, spanning…

In the last decade a number of rapidly evolving transients have been discovered that are not easily explained by traditional supernovae models. We present optical and UV data on onee such object, SN 2018gep, that displayed a fast rise with…

From the first two seasons of the Palomar Transient Factory, we identify three peculiar transients (PTF09dav, PTF10iuv, PTF11bij) with five distinguishing characteristics: peak luminosity in the gap between novae and supernovae (M_R = 15.5…

We present ongoing radio observations of the tidal disruption event (TDE) AT2018hyz, which was first detected in the radio at 972 days after disruption, following multiple non-detections from earlier searches. The new observations presented…

More than 100 tidal disruption events (TDEs) have been detected at multi-bands, which can be viewed as extreme laboratories to investigate the accretion physics and gravity in the immediate vicinity of massive black holes. Future transient…

High Energy Astrophysical Phenomena · Physics 2024-01-26 Zhiwei Chen , Youjun Lu , Yunfeng Chen

In the coming years, surveys such as the Rubin Observatory's Legacy Survey of Space and Time (LSST) are expected to increase the number of observed Tidal Disruption Events (TDEs) substantially. We employ Monte Carlo integration to calculate…

High Energy Astrophysical Phenomena · Physics 2026-01-16 E. Mamuzic , T. Ryu , S. H. Suyu , K. Szekerczes , S. Huber , L. Dai , M. Oguri

We present observations of four rapidly rising (t_{rise}~10d) transients with peak luminosities between those of supernovae (SNe) and superluminous SNe (M_{peak}~-20) - one discovered and followed by the Palomar Transient Factory (PTF) and…

The proximity and duration of the tidal disruption event (TDE) ASASSN-14li led to the discovery of narrow, blue-shifted absorption lines in X-rays and UV. The gas seen in X-ray absorption is consistent with bound material close to the…

High Energy Astrophysical Phenomena · Physics 2023-08-23 J. M. Miller , B. Mockler , E. Ramirez-Ruiz , P. A. Draghis , J. J. Drake , J. Raymond , M. T. Reynolds , X. Xiang , S. -B. Yun , A. Zoghbi

AT2018cqh is a unique optical tidal disruption event (TDE) discovered in a dwarf galaxy exhibiting delayed X-ray and radio flares. We present the results from high-resolution VLBA and e-MERLIN radio observations of AT2018cqh extending to…

High Energy Astrophysical Phenomena · Physics 2025-09-29 Lei Yang , Xinwen Shu , Guobin Mou , Yongquan Xue , Luming Sun , Fabao Zhang , Zhumao Zhang , Yibo Wang , Tao Wu , Ning Jiang , Hucheng Ding , Tinggui Wang

Observations of five Y dwarfs with three optical and near-infrared instruments at the 10.4 m Gran Telescopio Canarias are reported. Deep images of the five targets and a low-resolution far-red optical spectrum for one of the targets were…

Solar and Stellar Astrophysics · Physics 2024-03-20 Eduardo L. Martín , Jerry J. -Y. Zhang , Honorio Lanchas , Nicolas Lodieu , Tarik Shahbaz , Yakiv V. Pavlenko

Luminous fast blue optical transients (LFBOTs) are a growing class of enigmatic energetic transients. They show fast rises and declines, high temperatures throughout their evolution, and non-thermal emission in radio and X-rays. Their power…

Radio emission from tidal disruption events (TDEs) originates from an interaction of an outflow with the super-massive black hole (SMBH) circum nuclear material (CNM). In turn, this radio emission can be used to probe properties of both the…

High Energy Astrophysical Phenomena · Physics 2021-10-29 Assaf Horesh , Itai Sfaradi , Rob Fender , David A. Green , David R. A. Williams , Joe Bright

In this Letter, we report the detection of soft X-ray time lags-i.e. variability in the softer photons lagging behind that in the harder photons-in seven XMM-Newton observations of the tidal disruption event (TDE) candidate AT2021ehb. We…

High Energy Astrophysical Phenomena · Physics 2026-01-21 Wenjie Zhang

Type-IIn supernovae (SNe), which are characterized by strong interaction of their ejecta with the surrounding circumstellar matter (CSM), provide a unique opportunity to study the mass-loss history of massive stars shortly before their…

We present the discovery of a nuclear transient with the Caltech-NRAO Stripe 82 Survey (CNSS), a dedicated radio transient survey carried out with the Karl G. Jansky Very Large Array (VLA). This transient, CNSS J001947.3+003527, exhibited a…

High Energy Astrophysical Phenomena · Physics 2020-11-18 M. M. Anderson , K. P. Mooley , G. Hallinan , D. Dong , E. S. Phinney , A. Horesh , S. Bourke , S. B. Cenko , D. Frail , S. R. Kulkarni , S. Myers