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20082026
most citedIntermediate mass black holes in AGN disks: I. Production & Growth

355 citations · 1.6k across the 42 of their papers we have counts for

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9 papers · 1 filter

astro-ph.SR2026★ 3 cited

The bound origin of low-mass stellar binaries

A. Generozov, S. S. R. Offner, K. M. Kratter +3

Most main sequence stars, unlike our Sun, belong to multiple systems with two or more stars. How and when these multiples come together and become bound is uncertain, since the ear…

astro-ph.SR2025

The Single-Degenerate Channel Leads to Type Iax and Not Type Ia Supernovae due to Premature Ignition

Amir Michaelis, Hagai B. Perets

Type Ia supernovae (SNe Ia) are a critical tool for cosmology and galactic enrichment, yet the progenitor systems of normal SNe Ia remain a central puzzle. The long-debated single-…

astro-ph.SR2025★ 9 cited

An interferometric study of B star multiplicity

A. J. Frost, H. Sana, J-B Le Bouquin +7

Massive stars can have extreme effects on their environments from local to galactic scales. While O star multiplicity has been studied over a broad separation range (to the point w…

astro-ph.SR2023★ 16 cited

A Triple Scenario for the Formation of Wide Black Hole Binaries Such As Gaia BH1

A. Generozov, H. B. Perets

Recently, several non-interacting black hole-stellar binaries have been identified in Gaia data. For example, Gaia BH1, where a Sun-like star is in a moderate eccentricity (e=0.44)…

astro-ph.SR2022★ 22 cited

Hyper-runaway and hypervelocity white dwarf candidates in \textit{Gaia} Data Release 3: possible remnants from Ia/Iax supernova explosions or dynamical encounters

Andrei P. Igoshev, Hagai Perets, Na'ama Hallakoun

Type Ia and other peculiar supernovae (SNe) are thought to originate from the thermonuclear explosions of white dwarfs (WDs). Some of the proposed channels involve the ejection of…

astro-ph.SR2022★ 19 cited

3D Hydrodynamical Simulations of Helium-Ignited Double-degenerate White Dwarf Mergers

Niranjan Roy, Vishal Tiwari, Alexey Bobrick +6

The origins of type Ia supernovae (SNe Ia) are still debated. Some of the leading scenarios involve a double detonation in double white dwarf (WD) systems. In these scenarios, heli…

astro-ph.SR2022★ 5 cited

Compact objects formation, retention, and growth through accretion onto gas-embedded white-dwarfs/neutron-stars in gas-enriched globular-clusters

Hagai B. Perets

Observations of pulsars in globular clusters (GCs) give evidence that more >10-20% of neutron stars (NSs) ever formed in GCs were retained there. However, the velocity distribution…

astro-ph.SR2021★ 67 cited

Thermonuclear explosion of a massive hybrid HeCO white-dwarf triggered by a He-detonation on a companion

Ruediger Pakmor, Yossef Zenati, Hagai B. Perets +1

Normal type Ia supernovae (SNe) are thought to arise from the thermonuclear explosion of massive ( M) carbon-oxygen white dwarfs (WDs), although the exact mechanism i…

astro-ph.SR2012★ 65 cited

The Origins of Blue Stragglers and Binarity in Globular Clusters

Nathan Leigh, Christian Knigge, Alison Sills +3

(abridged) We use newly available empirical binary fractions for globular clusters to carry out a direct test of the binary evolution hypothesis, and of collisional channels that i…