activity
20242026
collaborators

8 papers

astro-ph.GA2026

Stellar mergers and chemical element mixing: implications for the metamorphic stellar evolution in AGN disks

Yanlong Shi, Xiaoshan Huang, Douglas N. C. Lin +1

Chemical mixing during stellar mergers can significantly influence the subsequent evolution of the merger remnant. We perform a suite of three-dimensional hydrodynamical simulation…

astro-ph.HE2026

The Light Curve of Wind-Reprocessed Tidal Disruption Events

Brenna Mockler, David Khatami, Daniel Kasen +2

The source of the optical/UV emission in tidal disruption events (TDEs) remains an enduring question in the field. Connecting the observed emission to the source is critical for bo…

astro-ph.HE2026

AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events

Yuhan Yao, Ryan Chornock, Andrew Mummery +39

We study AT2024kmq and AT2024lhc, two tidal disruption events (TDEs) with blue featureless spectra associated with high-mass black holes (). Both even…

astro-ph.HE2025

X-ray Variability and Photosphere Evolution during Accretion Disk Formation in Tidal Disruption Events

Xiaoshan Huang, Maria Renee Meza, Sol Bin Yun +3

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.…

astro-ph.HE2025

The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the X-rays and Radio

A. J. Nayana, Raffaella Margutti, Eli Wiston +34

We present X-ray (0.3--79 keV) and radio (0.25--203 GHz) observations of the most luminous Fast Blue Optical Transient (LFBOT) AT\,2024wpp at , spanning 2--280 days after…

astro-ph.HE2025

Perturbing AGN Accretion Disks with Stars and Moderately Massive Black Holes: Implications for Changing-Look AGN and Quasi-Periodic Eruptions

Sierra A. Dodd, Xiaoshan Huang, Shane W. Davis +1

We present a model that explains some extreme variability phenomena observed in active galactic nuclei (AGN). In this model, an orbiting companion interacts with the accretion disk…