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CSS J102913+404220 is a peculiar narrow line Seyfert 1 galaxy with an energetic nuclear optical outburst. We present a detailed analysis of its multi-wavelength photometric and spectroscopic observations covering a period of decade since…

High Energy Astrophysical Phenomena · Physics 2022-04-27 W. J. Zhang , X. W. Shu , Z. F. Sheng , L. M. Sun , L. M. Dou , N. Jiang , J. G. Wang , X. Y. Hu , Y. B. Wang , T. G. Wang

A tidal disruption event (TDE), AT2019dsg, was observed to be associated with a PeV neutrino event, IceCube-191001A, lagging the optical outburst by a half year. It is known that TDEs may generate ultrafast outflows. If the TDE occurs in a…

High Energy Astrophysical Phenomena · Physics 2022-06-22 Han-Ji Wu , Guo-Bin Mou , Kai Wang , Wei Wang , Zhuo Li

Recently, three optical tidal disruption event (TDE) candidates discovered by the Zwicky Transient Facility (ZTF) have been suggested to be coincident with high-energy neutrinos. They all exhibit unusually strong dust infrared (IR) echoes,…

High Energy Astrophysical Phenomena · Physics 2023-08-22 Ning Jiang , Ziying Zhou , Jiazheng Zhu , Yibo Wang , Tinggui Wang

The multiwavelength data of nuclear transient AT2018dyk, initially discovered as a changing-look low-ionization nuclear emission-line region (LINER) galaxy, has been revisited by us and found being in agreement with a tidal disruption event…

High Energy Astrophysical Phenomena · Physics 2023-09-04 Shifeng Huang , Ning Jiang , Zheyu Lin , Jiazheng Zhu , Tinggui Wang

One of the most prominent problems of optical/ultraviolet (UV) tidal disruption events (TDEs) is the origin of their optical/UV emission. It has been proposed that the soft X-rays produced by the stellar debris accretion disk can be…

High Energy Astrophysical Phenomena · Physics 2022-08-09 De-Fu Bu , Erlin Qiao , Xiao-Hong Yang , Jifeng Liu

Energetic nuclear outbursts have been discovered in luminous and ultraluminous infrared galaxies (U/LIRGs) at unexpectedly high rates. To investigate this population of transients, we performed a search in mid-IR data from the Wide-field…

Astrophysics of Galaxies · Physics 2022-10-12 T. M. Reynolds , S. Mattila , E. Kankare , A. Efstathiou , E. Kool , S. Ryder , L. Peña-Moñino , M. A. Pérez-Torres

Tidal disruption events (TDEs) are bursts of electromagnetic energy released when supermassive black holes (SMBHs) at the centers of galaxies violently disrupt a star that passes too close. TDEs provide a new window to study accretion onto…

Accretion at super-Eddington rates is expected to be accompanied by strong outflows. Such outflows are observed in Galactic X-ray binaries and extragalactic Ultra-luminous X-ray sources (ULXs). However, due to their large source distances,…

Ultraviolet (UV) observations of Type Ia supernovae (SNe Ia) are useful tools for understanding progenitor systems and explosion physics. In particular, UV spectra of SNe Ia, which probe the outermost layers, are strongly affected by the…

High Energy Astrophysical Phenomena · Physics 2018-06-13 Y. -C. Pan , R. J. Foley , A. V. Filippenko , N. P. M. Kuin

Tidal disruption events are routinely discovered as bright optical/UV flares, the properties of which are now well categorized on the population level. The underlying physical processes that produce the evolution of their X-ray emission and…

High Energy Astrophysical Phenomena · Physics 2025-12-11 Andrew Mummery , Brian Metzger , Sjoert van Velzen , Muryel Guolo

The James Webb Space Telescope (JWST) has recently uncovered the presence of low-luminosity active galactic nuclei (AGNs) at $z=4-11$. Spectroscopic observations have provided estimates of the nuclear black hole (BH) masses for these…

Astrophysics of Galaxies · Physics 2024-09-13 Kohei Inayoshi , Kazumi Kashiyama , Wenxiu Li , Yuichi Harikane , Kohei Ichikawa , Masafusa Onoue

Nuclear star clusters (NSCs), made up of a dense concentrations of stars and the compact objects they leave behind, are ubiquitous in the central regions of galaxies, surrounding the central supermassive black hole (SMBH). Close…

High Energy Astrophysical Phenomena · Physics 2024-03-28 Taeho Ryu , Rosalba Perna , Matteo Cantiello

We analyze 168 Swift monitoring observations of the nearest broad absorption line quasar Mrk 231 in the UV and X-ray bands, where we detect significant variability in the UV ($\sim$2246\AA) light curve with a null probability of…

Astrophysics of Galaxies · Physics 2018-08-29 Lilan Yang , Xinyu Dai , Youjun Lu , Zong-Hong Zhu , Francesco Shankar

The Swift satellite will be a self-contained observatory that will bring new capabilities to the observing of the early afterglow emission of Gamma-ray Bursts. Swift is completely autonomous and will do all of the observations without help…

We have observed four low-luminosity active galactic nuclei classified as Type 1 LINERs with the X-ray Telescope (XRT) and the UltraViolet-Optical Telescope (UVOT) onboard Swift, in an attempt to clarify the main powering mechanism of this…

High Energy Astrophysical Phenomena · Physics 2015-05-14 Elena Pian , Patrizia Romano , Dan Maoz , Antonino Cucchiara , Claudio Pagani , Valentina La Parola

The black-hole binary V404 Cyg entered the outburst phase in June 2015 after 26 years of X-ray quiescence, and with its behaviour broke the outburst evolution pattern typical of most black-hole binaries. We observed the entire outburst with…

AT 2019avd is a nuclear transient detected from infrared to soft X-rays, though its nature is yet unclear. The source has shown two consecutive flaring episodes in the optical and the infrared bands and its second flare was covered by X-ray…

Using archival SDSS multi-epoch imaging data (Stripe 82), we have searched for the tidal disruption of stars by super-massive black holes in non-active galaxies. Two candidate tidal disruption events (TDEs) are identified. They have optical…

Cosmology and Nongalactic Astrophysics · Physics 2012-07-23 Sjoert van Velzen , Glennys R. Farrar , Suvi Gezari , Nidia Morrell , Dennis Zaritsky , Linda Ostman , Mathew Smith , Joseph Gelfand , Andrew J. Drake

We present an analysis of over 150 ks of data on the planetary nebula WeBo 1 (PN G135.6+01.0) obtained with the Swift Ultraviolet Optical Telescope (UVOT). The central object of this nebula has previously been described as a late-type K…

Solar and Stellar Astrophysics · Physics 2015-06-05 Michael H. Siegel , Erik Hoversten , Howard E. Bond , Michele Stark , Alice A. Breeveld
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