After a star has been tidally disrupted by a black hole, the debris forms an elongated stream.
We start by studying the evolution of this gas before its bound part returns to the original …

A tidal disruption event (TDE) ensues when a star passes too close to a supermassive black
hole (SMBH) in a galactic center, and is ripped apart by its tidal field. The gaseous debris …

Theoretical modeling of massive stars predicts a gap in the black hole (BH) mass function
above∼ 40–50 M⊙ for BHs formed through single star evolution, arising from (pulsational) …

The gravitational-wave astronomical revolution began in 2015 with LIGO's observation of the
coalescence of two stellar-mass black holes. Over the coming decades, ground-based …

We study how the matter dispersed when a supermassive black hole tidally disrupts a star
joins an accretion flow. Combining a relativistic hydrodynamic simulation of the stellar …

The majority of long-duration (> 2 s) gamma-ray bursts (GRBs) arise from the collapse of
massive stars, with a small proportion created from the merger of compact objects. Most of …

The tidal disruption of a star by a massive black hole is expected to yield a luminous flare of
thermal emission. About two dozen of these stellar tidal disruption flares (TDFs) may have …

Abstract Using the Zwicky Transient Facility alert stream, we are conducting a large
spectroscopic campaign to construct a complete, volume-limited sample of transients …

Main-sequence disruptions of stars by supermassive black holes result in the production of
an extended, geometrically thin debris stream winding repeatedly around the black hole. In …

Quasi-periodic eruptions (QPEs) are found in the center of five galaxies, where a tidal
disruption event (TDE)-like event has been reported in GSN 069, which occurred a couple of …