activity
20172026
most citedCommon Envelope Wind Tunnel: Coefficients of Drag and Accretion in a Simplified Context for Studying Flows Around Objects Embedded Within Stellar Envelopes

113 citations · 401 across the 14 of their papers we have counts for

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Showing astro-ph.HEShow all

7 papers · 1 filter

astro-ph.HE2026

The rise of the black hole X-ray binary AT2019wey observed with TESS

Alyana Jusino, Kishalay De, Andrea Antoni

Black hole X-ray binaries (BHXRBs) have traditionally been discovered by X-ray surveys with cadences of hours to days. However, large optical time-domain surveys now provide novel…

astro-ph.HE2024★ 5 cited

Disappearance of a massive star in the Andromeda Galaxy due to formation of a black hole

Kishalay De, Morgan MacLeod, Jacob E. Jencson +11

When a massive star reaches the end of its lifetime, its core collapses and releases neutrinos that drive a shock into the outer layers (stellar envelope). A sufficiently strong sh…

astro-ph.HE2023★ 35 cited

Numerical simulations of the random angular momentum in convection II: delayed explosions of red supergiants following "failed'' supernovae

Andrea Antoni, Eliot Quataert

When collapse of the iron core in a massive red or yellow supergiant does not lead to an energetic supernova, a significant fraction of the convective hydrogen envelope will fall i…

astro-ph.HE2021★ 1 cited

Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes

Andrea Antoni, Eliot Quataert

During the core collapse of massive stars that do not undergo a canonical energetic explosion, some of the hydrogen envelope of a red supergiant (RSG) progenitor may infall onto th…

astro-ph.HE2021★ 30 cited

The hydrodynamic evolution of binary black holes embedded within the vertically stratified disks of active galactic nuclei

Nicholas Kaaz, Sophie Lund Schrøder, Jeff J. Andrews +2

Stellar-mass black holes can become embedded within the gaseous disks of active galactic nuclei (AGNs). Afterwards, their interactions are mediated by their gaseous surroundings. I…

astro-ph.HE2019★ 58 cited

The Evolution of Binaries in a Gaseous Medium: Three-Dimensional Simulations of Binary Bondi-Hoyle-Lyttleton Accretion

Andrea Antoni, Morgan MacLeod, Enrico Ramirez-Ruiz

Binary stars are common. While only those with small separations may exchange gas with one another, even the widest binaries interact with their gaseous surroundings. Drag forces a…

astro-ph.HE2019★ 23 cited

Bondi-Hoyle-Lyttleton Accretion onto Star Clusters

Nicholas Kaaz, Andrea Antoni, Enrico Ramirez-Ruiz

An isolated star moving supersonically through a uniform gas accretes material from its gravitationally-induced wake. The rate of accretion is set by the accretion radius of the st…