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From the 2 of 23 linked papers with an AI index.

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20242026
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astro-ph.HE2024

Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries

Camille Liotine, Vicky Kalogera, Jeff J. Andrews +12

Binaries harboring a millisecond pulsar (MSP) and a black hole (BH) are a key observing target for current and upcoming pulsar surveys. We model the formation and evolution of such…

astro-ph.SR2024

Mass Transfer in Eccentric Orbits with Self-consistent Stellar Evolution

Kyle Akira Rocha, Rachel Hur, Vicky Kalogera +12

We investigate Roche lobe overflow mass transfer (MT) in eccentric binary systems between stars and compact objects (COs), modeling the coupled evolution of both the star and the o…

astro-ph.SR2024

Irregularly Sampled Time Series Interpolation for Detailed Binary Evolution Simulations

Philipp M. Srivastava, Ugur Demir, Aggelos Katsaggelos +14

Modeling of large populations of binary stellar systems is an intergral part of a many areas of astrophysics, from radio pulsars and supernovae to X-ray binaries, gamma-ray bursts,…

astro-ph.SR2024

The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars

Matthias U. Kruckow, Jeff J. Andrews, Tassos Fragos +10

Context. The black holes discovered using Gaia, especially Gaia BH1 and BH2, have low mass companions of solar-like metallicity in wide orbits. For standard isolated binary evoluti…

astro-ph.SR2024

The effect of mass loss in models of red supergiants in the Small Magellanic Cloud

E. Zapartas, S. de Wit, K. Antoniadis +16

The rate and mechanism of mass loss of red supergiants (RSGs) remain poorly understood, especially at low metallicities. Motivated by the new empirical prescription by Yang et al.…

astro-ph.HE2024

Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation

Zepei Xing, Tassos Fragos, Emmanouil Zapartas +12

The three dynamically confirmed wind-fed black hole high-mass X-ray binaries (BH-HMXBs) are suggested to all contain a highly spinning black hole (BH). However, based on the theori…