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Theoretical expectations for high-mass X-ray binaries, supernova remnants, and their evolutionary paths: An overview talk for LIAC41: the eventful life of stellar multiples

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arxiv 2410.07747 v2 pith:OWOXIX45 submitted 2024-10-10 astro-ph.HE astro-ph.SR

Ilya Mandel This is my paper · ORCID
classification astro-ph.HEastro-ph.SR
keywords binarieseventfulevolutionaryhigh-masslifemultiplespathsstellar
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In this invited talk at the 41st Li\`ege International Astrophysical Colloquium on "The eventful life of massive star multiples", I reviewed some aspects of our current understanding of neutron stars and black holes as end products of stellar evolution as well as the evolutionary paths leading to the formation of high-mass X-ray binaries.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. On Neutron Star Natal Kicks in High-Mass X-Ray Binaries: Insights from Population Synthesis

    astro-ph.HE 2025-04 conditional novelty 5.0 of 10

    From 36 neutron-star X-ray binaries, the best-fitting natal kick model is a bimodal Maxwellian with sigma=320 km/s for core-collapse supernovae and sigma=80 km/s for electron-capture supernovae.

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