English
Related papers

Related papers: Accretion disc cooling and narrow absorption lines…

200 papers

Tidal disruption events (TDEs) show a correlation between the UV to X-ray spectral index and the Eddington ratio, with non-thermal X-ray emission at the low Eddington ratio. We consider the corona surrounding the accretion disc as a…

High Energy Astrophysical Phenomena · Physics 2022-11-30 T. Mageshwaran , Sudip Bhattacharyya

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…

High Energy Astrophysical Phenomena · Physics 2017-12-27 S. Gezari , S. B. Cenko , I. Arcavi

Quasi-periodic eruptions (QPEs) are X-ray transients characterized by nearly regular recurring flares from galactic nuclei. Recent observations have confirmed that some QPEs occur in galactic centers that experienced a tidal disruption…

High Energy Astrophysical Phenomena · Physics 2025-12-09 Tomoya Suzuguchi , Tatsuya Matsumoto

A star crossing the tidal radius of a supermassive black hole will be spectacularly ripped apart with an accompanying burst of radiation. A few tens of such tidal disruption events (TDEs) have now been identified in the optical wavelengths,…

We present light curves and spectra of the tidal disruption event (TDE) ASASSN-18pg / AT 2018dyb spanning a period of one year. The event shows a plethora of strong emission lines, including the Balmer series, He II, He I and metal lines of…

This article provides a summary of XMM-Newton highlights on stellar tidal disruption events. First found with ROSAT, ongoing and upcoming sky surveys will detect these events in the 1000s. In X- rays, tidal disruption events (TDEs) provide…

High Energy Astrophysical Phenomena · Physics 2017-05-10 S. Komossa

We present the results from our multi-wavelength monitoring campaign of the transient AT2022wtn, discovered by the Zwicky Transient Facility in the nucleus of SDSSJ232323.79+104107.7, the less massive galaxy in an active merging pair with a…

When a star passes through the tidal disruption radius of a massive black hole (BH), it can be torn apart by the tidal force of the BH, known as the Tidal Disruption Event (TDE). Since the observed UV/optical luminosity significantly…

High Energy Astrophysical Phenomena · Physics 2025-01-17 Hengxiao Guo , Jingbo Sun , Shuang-Liang Li , Yan-Fei Jiang , Tinggui Wang , Defu Bu , Ning Jiang , Yanan Wang , Yuhan Yao , Rongfeng Shen , Minfeng Gu , Mouyuan Sun

Tidal disruption events (TDEs), which occur when stars enter the tidal radii of supermassive black holes (SMBHs) and are subsequently torn apart by their tidal forces, represent intriguing phenomena that stimulate growing research interest…

Tidal disruption events (TDEs) can uncover the quiescent black holes (BHs) at the center of galaxies and also offer a promising method to study them. In a partial TDE (PTDE), the BH's tidal force cannot fully disrupt the star, so the…

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

We report on the SRG/eROSITA detection of ultra-soft ($kT=47^{+5}_{-5}$ eV) X-ray emission ($L_{\mathrm{X}}=2.5^{+0.6}_{-0.5} \times 10^{43}$ erg s$^{-1}$) from the tidal disruption event (TDE) candidate AT 2022dsb $\sim$14 days before peak…

High Energy Astrophysical Phenomena · Physics 2023-09-29 A. Malyali , A. Rau , C. Bonnerot , A. J. Goodwin , Z. Liu , G. E. Anderson , J. Brink , D. A. H. Buckley , A. Merloni , J. C. A. Miller-Jones , I. Grotova , A. Kawka

A Tidal Disruption Event (TDE) occurs when a supermassive black hole tidally disrupt a nearby passing star. The fallback accretion rate of the disrupted star may exceed the Eddington limit, which induces a supersonic outflow and a burst of…

High Energy Astrophysical Phenomena · Physics 2023-09-14 Zsófia V. Kovács-Stermeczky , József Vinkó

The early time emission in tidal disruption events (TDEs) originates from both accretion and shocks, which produce photons that eventually emerge from an inhomogeneous photosphere. In this work, we model the disk formation following the…

High Energy Astrophysical Phenomena · Physics 2025-12-16 Xiaoshan Huang , Maria Renee Meza , Sol Bin Yun , Brenna Mockler , Shane W. Davis , Yan-fei Jiang

Quasi-periodic eruptions (QPEs) are recurring soft X-ray transients emerging from the vicinity of supermassive black holes (SMBHs) in nearby, low-mass galaxy nuclei; about ten QPE hosts have been identified thus far. Here we report the…

Tidal disruption events (TDEs) occur when a star passes close enough to a galaxy's supermassive black hole to be disrupted by tidal forces. We discuss new observations of IGRJ12580+0134, a TDE observed in NGC 4845 (d=17 Mpc) in November…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Eric S. Perlman , Eileen T. Meyer , Q. Daniel Wang , Qiang Yuan , Richard Henriksen , Judith Irwin , Jiangtao Li , Theresa Wiegert , Haochuan Li

The tidal disruption event (TDE) AT2022cmc represents the fourth known example of a relativistic jet produced by the tidal disruption of a stray star providing a unique probe of the formation and evolution of relativistic jets in otherwise…

High Energy Astrophysical Phenomena · Physics 2024-12-31 T. Eftekhari , A. Tchekhovskoy , K. D. Alexander , E. Berger , R. Chornock , T. Laskar , R. Margutti , Y. Yao , Y. Cendes , S. Gomez , A. Hajela , D. R. Pasham

Tidal disruption events\,(TDEs) provide a valuable probe in studying the dynamics of stars in the nuclear environments of galaxies. Recent observations show that TDEs are strongly overrepresented in post-starburst or "green valley"…

High Energy Astrophysical Phenomena · Physics 2024-01-01 Mengye Wang , Yiqiu Ma , Qingwen Wu , Ning Jiang

Tidal disruption events (TDEs) are multi-messenger transients in which a star is tidally destroyed by a supermassive black hole at the center of galaxies. The Rubin Observatory Legacy Survey of Space and Time (LSST) is anticipated to…

High Energy Astrophysical Phenomena · Physics 2024-10-30 K. Szekerczes , T. Ryu , S. H. Suyu , S. Huber , M. Oguri , L. Dai

We consider Roche lobe overflow (RLO) from a low-mass star on a nearly circular orbit, onto a supermassive black hole (SMBH). If mass transfer is unstable, its rate accelerates in a runaway process, resulting in highly super-Eddington mass…

High Energy Astrophysical Phenomena · Physics 2024-07-02 Itai Linial , Eliot Quataert
‹ Prev 1 4 5 6 7 8 10 Next ›