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ASASSN-14li is a low-redshift ($z= 0.0206$) tidal disruption event (TDE) that has been studied extensively across the entire electromagnetic spectrum, and has provided one of the most sensitive measurements of a TDE to-date. Its X-ray…

高能天体物理现象 · 物理学 2024-01-24 Yukta Ajay , Dheeraj R. Pasham , Thomas Wevers , Eric R. Coughlin , Francesco Tombesi , Muryel Guolo , James F. Steiner

Tidal disruption events (TDEs) are exotic transients that can lead to temporary super-Eddington accretion onto a supermassive black hole. Such accretion mode is naturally expected to result in powerful outflows of ionized matter. However,…

高能天体物理现象 · 物理学 2023-08-11 P. Kosec , D. Pasham , E. Kara , F. Tombesi

We report the discovery of transient radio emission from the nearby optically-discovered TDE ASASSN-14li (distance of 90 Mpc), making it the first typical TDE detected in the radio, and unambiguously pointing to the formation of a…

高能天体物理现象 · 物理学 2016-03-16 Kate D. Alexander , Edo Berger , James Guillochon , Bevin A. Zauderer , Peter K. G. Williams

ASASSN-14li is a recently-discovered tidal disruption event with an exceptionally rich data-set: spectra and lightcurves in soft X-rays, UV, optical, and radio. To understand its emission properties in all these bands, we have extended our…

高能天体物理现象 · 物理学 2016-08-24 Julian Krolik , Tsvi Piran , Gilad Svirski , Roseanne M. Cheng

We present ground-based and Swift photometric and spectroscopic observations of the candidate tidal disruption event (TDE) ASASSN-14li, found at the center of PGC 043234 ($d\simeq90$ Mpc) by the All-Sky Automated Survey for SuperNovae…

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…

高能天体物理现象 · 物理学 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

We present late-time optical spectroscopy and X-ray, UV, and optical photometry of the nearby ($d=214$ Mpc, $z=0.0479$) tidal disruption event (TDE) ASASSN-15oi. The optical spectra span 450 days after discovery and show little remaining…

高能天体物理现象 · 物理学 2019-10-14 T. W. -S. Holoien , J. S. Brown , K. Auchettl , C. S. Kochanek , J. L. Prieto , B. J. Shappee , J. Van Saders

Supermassive black holes can experience super-Eddington peak mass fallback rates following the tidal disruption of a star. The theoretical expectation is that part of the infalling material is expelled by means of an accretion disk wind,…

高能天体物理现象 · 物理学 2024-01-09 T. Wevers , M. Guolo , D. R. Pasham , E. R. Coughlin , F. Tombesi , Y. Yao , S. Gezari

We present a Hubble Space Telescope STIS spectrum of ASASSN-14li, the first rest-frame UV spectrum of a tidal disruption flare (TDF). The underlying continuum is well fit by a blackbody with $T_{\mathrm{UV}} = 3.5 \times 10^{4}$ K, an order…

We report the detection and characterization of ultrafast outflows (UFOs) in the X-ray spectra of the tidal disruption event (TDE) AT2020afhd, based on observations from NICER, Swift, and XMM. Prominent blueshifted absorption features were…

高能天体物理现象 · 物理学 2025-07-22 Zikun Lin , Yanan Wang , De-Fu Bu , Junjie Mao , Jifeng Liu

We report European Very Long Baseline Interferometry Network (EVN) radio continuum observations of ASASSN-14li, one of the best studied tidal disruption events (TDEs) to date. At 1.7 GHz with ~12x6mas resolution, the emission is unresolved.…

We present late-time observations by Swift and XMM-Newton of the tidal disruption event (TDE) ASASSN-15oi that reveal that the source brightened in the X-rays by a factor of $\sim10$ one year after its discovery, while it faded in the…

高能天体物理现象 · 物理学 2017-12-27 S. Gezari , S. B. Cenko , I. Arcavi

We present late-time optical spectroscopy taken with the Large Binocular Telescope's Multi-Object Double Spectrograph, late-time SWIFT UVOT and XRT observations, as well as improved ASAS-SN pre-discovery limits on the nearby (d=90.3 Mpc,…

高能天体物理现象 · 物理学 2017-01-18 J. S. Brown , T. W. -S Holoien , K. Auchettl , K. Z. Stanek , C. S. Kochanek , B. J. Shappee , J. L. Prieto , D. Grupe

We report the detection of a significant infrared variability of the nearest tidal disruption event (TDE) ASASSN-14li using Wide-field Infrared Survey Explorer} and newly released Near-Earth Object WISE Reactivation} data. In comparison…

高能天体物理现象 · 物理学 2016-09-08 Ning Jiang , Liming Dou , Tinggui Wang , Chenwei Yang , Jianwei Lyu , Hongyan Zhou

We present ground-based and Swift photometric and spectroscopic observations of the tidal disruption event (TDE) ASASSN-15oi, discovered at the center of 2MASX J20390918-3045201 ($d\simeq216$ Mpc) by the All-Sky Automated Survey for…

ASASSN-14ae is a candidate tidal disruption event (TDE) found at the center of SDSS J110840.11+340552.2 ($d\simeq200$~Mpc) by the All-Sky Automated Survey for Supernovae (ASAS-SN). We present ground-based and Swift follow-up photometric and…

The ultrasoft X-ray flare 2XMMi J184725.1-631724 was serendipitously detected in two XMM-Newton observations in 2006 and 2007, with a peak luminosity of 6X10^43 erg/s. It was suggested to be a tidal disruption event (TDE) because its…

高能天体物理现象 · 物理学 2017-12-27 Dacheng Lin , Jay Strader , Eleazar R. Carrasco , Olivier Godet , Dirk Grupe , Natalie A. Webb , Didier Barret , Jimmy A. Irwin

We have discovered an ultrasoft X-ray transient source, 2XMMi J184725.1-631724, which was detected serendipitously in two XMM-Newton observations in the direction of the center of the galaxy IC 4765-f01-1504 at a redshift of 0.0353. These…

高能天体物理现象 · 物理学 2015-05-28 Dacheng Lin , Eleazar R. Carrasco , Dirk Grupe , Natalie A. Webb , Didier Barret , Sean A. Farrell

We present radio observations of the tidal disruption event candidate (TDE) XMMSL1 J0740$-$85 spanning 592 to 875 d post X-ray discovery. We detect radio emission that fades from an initial peak flux density at 1.6 GHz of $1.19\pm 0.06$ mJy…

高能天体物理现象 · 物理学 2017-03-22 K. D. Alexander , M. H. Wieringa , E. Berger , R. D. Saxton , S. Komossa
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