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Rates and environments of neutron star binaries

Published online by Cambridge University Press:  27 February 2023

Irina Dvorkin Open the ORCID record for Irina Dvorkin [Opens in a new window]
Irina Dvorkin*
Affiliation:
Institut d’Astrophysique de Paris, Sorbonne Université & CNRS, UMR 7095, 98 bis bd Arago, F-75014 Paris, France
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Abstract

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Recent observations of the various phases in the lives of neutron star binaries across different messengers have led to major discoveries and raised new exciting questions about the environments of these systems. We will overview the current observational constraints on the formation rates and environments of neutron star binaries, as well as theoretical predictions that will be confronted with future observations.

Keywords

stars: neutronbinaries
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S363: Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution , June 2020 , pp. 33 - 42
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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