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Related papers: An intermediate-luminosity-optical-transient (ILOT…

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When a star passes within the tidal radius of a supermassive black hole, it will be torn apart. For a star with the mass of the Sun ($M_\odot$) and a non-spinning black hole with a mass $<10^8 M_\odot$, the tidal radius lies outside the…

We show that a Quark-Nova (QN; the explosive transition of a neutron star to a quark star) occurring a few days following the supernova explosion of an Oxygen-type Wolf-Rayet (WO) star can account for the intriguing features of ASASSN-15lh,…

High Energy Astrophysical Phenomena · Physics 2016-11-14 Rachid Ouyed , Denis Leahy , Luis Welbanks , Nico Koning

We present optical spectroscopy, ultraviolet to infrared imaging and X-ray observations of the intermediate luminosity optical transient (ILOT) SN 2010da in NGC 300 (d=1.86 Mpc) spanning from -6 to +6 years relative to the time of outburst…

[abridged] We present multi-epoch high-resolution optical spectroscopy, UV/radio/X-ray imaging, and archival Hubble and Spitzer observations of an intermediate luminosity optical transient recently discovered in the nearby galaxy NGC300. We…

Planets grow in rotating disks of dust and gas around forming stars, some of which can subsequently collide in giant impacts after the gas component is removed from the disk. Monitoring programs with the warm Spitzer mission have recorded…

We model the optical and infrared transient ZTF SLRN-2020, previously associated with a star-planet merger. We consider the scenario in which orbital decay via tidal dissipation led to the merger, and find that tidal heating within the star…

High Energy Astrophysical Phenomena · Physics 2025-12-12 Ricardo Yarza , Morgan MacLeod , Benjamin Idini , Ruth Murray-Clay , Enrico Ramirez-Ruiz

The James Webb Space Telescope (JWST) has opened up a new window to study highly reddened explosive transients. We present results from late-time (1421 days post-explosion) JWST follow-up spectroscopic observations with NIRSpec and MIRI LRS…

Solar and Stellar Astrophysics · Physics 2024-07-31 Sam Rose , Ryan M. Lau , Jacob E. Jencson , Mansi M. Kasliwal , Kishalay De , Michael E. Ressler , Ori D. Fox , Matthew J. Hankins

Some transients, although classified as novae based on their maximum and early decline optical spectra, cast doubts on their true nature and whether nova impostors might exist. We monitored a candidate nova which displayed a distinctly…

Solar and Stellar Astrophysics · Physics 2020-03-25 Elena Mason , Steven N. Shore , Paul Kuin , Terry Bohlsen

A luminous optical transient (OT) that appeared in NGC 300 in early 2008 had a maximum brightness, M_V ~ -12 to -13, intermediate between classical novae and supernovae. We present ground-based photometric and spectroscopic monitoring and…

We suggest that in the rare case of an Intermediate-Luminosity Optical Transient (ILOTs) event, evaporation of extra-solar Kuiper belt objects (ExtraKBOs) at distances of d ~ 500 - 10000AU from the ILOT can be detected. If the ILOT lasts…

Solar and Stellar Astrophysics · Physics 2016-07-13 Ealeal Bear , Noam Soker

We present the detection of persistent soft X-ray radiation with L_x ~ 10^41-10^42 erg/s at the location of the extremely luminous, double-humped transient ASASSN-15lh as revealed by Chandra and Swift. We interpret this finding in the…

ASASSN-21qj is a distant Sun-like star that recently began an episode of deep dimming events after no prior recorded variability. Here we examine archival and newly obtained optical and near-infrared data of this star. The deep aperiodic…

We report the discovery of a new transiting exoplanet orbiting the star TIC~257060897 and detected using {\it TESS} full frame images. We acquired HARPS-N time-series spectroscopic data, and ground-based photometric follow-up observations…

Earth and Planetary Astrophysics · Physics 2021-10-20 M. Montalto , L. Malavolta , J. Gregorio , G. Mantovan , S. Desidera , G. Piotto , V. Nascimbeni , V. Granata , E. E. Manthopoulou , R. Claudi

We find that dust clouds which eclipse young stars obscure the stellar disc inhomogeneously. In the particular case of CQ Tau, we find isolated optically thick structures with sizes $\lesssim0.6R_*$ and derive the typical $A_{V}$ gradient…

Solar and Stellar Astrophysics · Physics 2021-06-23 A. V. Dodin , E. A. Suslina

Despite the success of discovering transiting exoplanets, several recently observed objects (e.g. KIC-8462852, J1407 and PDS-110) exhibit unconventional transit signals, whose appropriate interpretation in terms of a spherical single body…

Earth and Planetary Astrophysics · Physics 2019-12-02 Mario Sucerquia , Jaime A. Alvarado-Montes , Vanesa Ramírez , Jorge I. Zuluaga

Aims: AT 2018hso is a new transient showing transitional properties between those of LRNe and the class of intermediate luminosity red transients (ILRTs) similar to SN 2008S. Through the detailed analysis of the observed parameters, our…

We propose that the intermediate luminosity optical transient NGC 300 OT2008-1 was powered by a mass transfer episode from an extreme Asymptotic Giant Branch star to a Main Sequence companion. We find a remarkable similarity of the shapes…

Solar and Stellar Astrophysics · Physics 2015-05-14 Amit Kashi , Adam Frankowski , Noam Soker