More Like this

1. Tidal Disruptions of Main-sequence Stars. V. The Varieties of Disruptions

   https://doi.org/10.3847/1538-4357/abc0f6  

   Krolik, Julian; Piran, Tsvi; Ryu, Taeho (November 2020, The Astrophysical Journal)
2. Tidal Disruptions of Main-sequence Stars. III. Stellar Mass Dependence of the Character of Partial Disruptions

   https://doi.org/10.3847/1538-4357/abb3ce  

   Ryu, Taeho; Krolik, Julian; Piran, Tsvi; Noble, Scott C. (December 2020, The Astrophysical Journal)
3. Tidal Disruptions of White Dwarfs: Theoretical Models and Observational Prospects

   https://doi.org/10.1007/s11214-020-00661-2  

   Maguire, Kate; Eracleous, Michael; Jonker, Peter G.; MacLeod, Morgan; Rosswog, Stephan (April 2020, Space Science Reviews)
4. The most energetic transients: Tidal disruptions of high-mass stars

   https://doi.org/10.1126/sciadv.adt0074  

   Hinkle, Jason T; Shappee, Benjamin J; Auchettl, Katie; Kochanek, Christopher S; Neustadt, Jack_M M; Polin, Abigail; Strader, Jay; Holoien, Thomas W-S; Huber, Mark E; Tucker, Michael A; et al (June 2025, Science Advances)

   We present the class of extreme nuclear transients (ENTs), including the most energetic single transient yet found, Gaia18cdj. Each ENT is coincident with its host-galaxy nucleus and exhibits a smooth (<10% excess variability), luminous (2 × 10⁴⁵to 7 × 10⁴⁵erg per second), and long-lived (>150 days) flare. ENTs are extremely rare (≥1 × 10^–3cubic gigaparsec per year) compared to any other known class of transients. They are at least twice as energetic (0.5 × 10⁵³to 2.5 × 10⁵³erg) as any other known transient, ruling out supernova origins. Instead, the high peak luminosities, long flare timescales, and immense radiated energies of the ENTs are most consistent with the tidal disruption of high-mass (  $\gtrsim 3{\mathrm{M}}_{\odot }$ ) stars by massive (  $\gtrsim {10}^8 {\mathrm{M}}_{\odot }$ ) supermassive black holes (SMBHs). ENTs will be visible to high redshifts (z~ 4 to 6) in upcoming surveys, providing an avenue to study the high-mass end of the SMBH mass distribution, complementing recent studies of actively accreting SMBHs at high redshifts with the James Webb Space Telescope. 

   more » « less
5. Tidal Disruptions of Stars by Black Hole Remnants in Dense Star Clusters

   https://doi.org/10.3847/1538-4357/ab2e0c  

   Kremer, Kyle; Lu, Wenbin; Rodriguez, Carl L.; Lachat, Mitchell; Rasio, Frederic A. (August 2019, The Astrophysical Journal)