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Related papers: Dust Echoes from Luminous Fast Blue Optical Transi…

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SN2017hcc was remarkable for being a nearby and strongly polarized superluminous TypeIIn supernova (SN). We obtained high-resolution echelle spectra that we combine with other spectra to investigate its line profile evolution. All epochs…

High Energy Astrophysical Phenomena · Physics 2020-10-14 Nathan Smith , Jennifer E. Andrews

Luminous Fast Blue Optical Transients (LFBOTs) are rare extragalactic events of unknown origin. Tidal disruptions of white dwarfs by intermediate mass black holes (BHs), mergers of BHs and Wolf-Rayet stars, and failed supernovae are among…

High Energy Astrophysical Phenomena · Physics 2026-02-18 A. A. Chrimes , P. G. Jonker , A. J. Levan , A. Mummery

Newly-born, rapidly-spinning magnetars have been invoked as the power sources of super-luminous transients, including the class of "fast-luminous optical transients" (FBOTs). The extensive multi-wavelength analysis of AT2018cow, the first…

High Energy Astrophysical Phenomena · Physics 2019-06-19 Ke Fang , Brian D. Metzger , Kohta Murase , Imre Bartos , Kumiko Kotera

To determine the epoch of reionization precisely and to reveal the property of inhomogeneous reionization are some of the most important topics of modern cosmology. Existing methods to investigate reionization which use cosmic microwave…

High Energy Astrophysical Phenomena · Physics 2020-02-26 Tomoki Terasaki , Daichi Tsuna , Toshikazu Shigeyama

Massive stars (>8 $M_{\odot}$) often undergo intense mass loss through winds or eruptive events in the final stages of their evolution, leading to the formation of a dense circumstellar medium (CSM). This material, expelled months to years…

High Energy Astrophysical Phenomena · Physics 2025-10-15 Silvia Gagliardini , Simone Dall'Osso , Dafne Guetta , Angela Zegarelli , Silvia Celli , Antonio Capone , Irene Di Palma

I propose a new scenario, the polar common envelope jets supernova (CEJSN) impostor scenario, to account for AT2018cow-like fast blue optical transients (FBOTs). The polar CEJSN impostor scenario evolves through four main phases. (1) A red…

High Energy Astrophysical Phenomena · Physics 2022-05-04 Noam Soker

We present near-infrared (NIR) and optical observations and analysis of the Type Ibn/Icn supernova (SN) 2023xgo, spanning the period from two days to 100 days past explosion. A comparison of the NIR light curves and color evolution with…

High Energy Astrophysical Phenomena · Physics 2025-08-26 Masayuki Yamanaka , Takahiro Nagayama

We use a Monte Carlo radiative transfer model (MCRTM) to simulate the UBVRI light curves, images and linear polarization of a light echo from supernova SN$~$1987A in the Large Magellanic Cloud (LMC) using various dust cloud shapes, sizes,…

High Energy Astrophysical Phenomena · Physics 2021-10-04 Jiachen Ding , Lifan Wang , Peter Brown , Ping Yang

The discovery of SN 2018gep (ZTF18abukavn) challenged our understanding of the late-phase evolution of massive stars and their supernovae (SNe). The fast rise in luminosity of this SN (spectroscopically classified as a broad-lined Type Ic…

High Energy Astrophysical Phenomena · Physics 2021-10-20 Shing-Chi Leung , Jim Fuller , Ken'ichi Nomoto

A search for the progenitor of SN~2010jl, an unusually luminous core-collapse supernova of Type~IIn, using pre-explosion {\it Hubble}/WFPC2 and {\it Spitzer}/IRAC images of the region, yielded upper limits on the UV and near-infrared (IR)…

AT 2022cmc is a luminous optical transient ($\nu L_{\nu} \gtrsim 10^{45}$ erg s$^{-1}$) accompanied by decaying non-thermal X-rays (peak duration $t_{\rm X} \lesssim$ days and isotropic energy $E_{\rm X,iso} \gtrsim 10^{53}$ erg) and a…

High Energy Astrophysical Phenomena · Physics 2023-05-03 Tatsuya Matsumoto , Brian D. Metzger

AT 2020mot is a typical UV/optical tidal disruption event (TDE) with no radio or X-ray signatures in a quiescent host. We find an i-band excess and re-brightening along the decline of the light curve which could be due to two consecutive…

The progenitors of SN 2008S and the 2008 transient in NGC300 were dust-enshrouded, with extremely red mid-infrared (MIR) colors and relatively low luminosities. The transients were optically faint (-13 < M_V < -15) compared to normal…

Type IIn SNe show spectral evidence for strong interaction between their blast wave and dense circumstellar material (CSM) around the progenitor star. SN2010jl was the brightest core-collapse SN in 2010, and it was a Type IIn explosion with…

HST and ground based observations of the Type IIn SN 2010jl are analyzed, including photometry, spectroscopy in the ultraviolet, optical and NIR bands, 26-1128 days after first detection. At maximum the bolometric luminosity was $\sim…

We report unnoticed but intriguing features in the peculiar nuclear transient AT 2022fpx, and investigate its type. These features include the constantly red optical color of $g-r>0$, a stable soft X-ray flare ($kT\sim100$ eV) in the past…

High Energy Astrophysical Phenomena · Physics 2025-09-09 Zheyu Lin , Ning Jiang , Yibo Wang , Xu Kong , Shifeng Huang , Zesen Lin , Chen Qin , Tianyu Xia

SN2008S and the 2008 NGC300-OT were explosive transients of stars self-obscured by very dense, dusty stellar winds. An explosive transient with an un-observed shock break-out luminosity of order 10^10 Lsun is required to render the…

Solar and Stellar Astrophysics · Physics 2015-05-28 C. S. Kochanek

We report optical spectroscopic observations of four blue-excess dust-obscured galaxies (BluDOGs) identified by Subaru Hyper Suprime-Cam. BluDOGs are a sub-class of dust-obscured galaxies (DOGs, defined with the extremely red color…

AT 2018cow was the nearest and best studied example of a new breed of extra-galactic, luminous and rapidly-evolving transient. Both the progenitor systems and explosion mechanisms of these rapid transients remain a mystery - the energetics,…

Astrophysics of Galaxies · Physics 2020-05-27 J. D. Lyman , L. Galbany , S. F. Sanchez , J. P. Anderson , H. Kuncarayakti