The lifetime of binary neutron star merger remnants-Reference-Cited by-同舟云学术

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The lifetime of binary neutron star merger remnants

Published:2020-08 Issue: Volume:27 Page:33-37
ISSN:2214-4048
Container-title:Journal of High Energy Astrophysics
language:en
Short-container-title:Journal of High Energy Astrophysics

Author:

Lucca Matteo^ORCID,Sagunski Laura^ORCID

Funder

Natural Sciences and Engineering Research Council of Canada

Publisher

Elsevier BV

Subject

Astronomy and Astrophysics,Space and Planetary Science

Reference51 articles.

1. Observation of gravitational waves from a binary black hole merger;Abbott;Phys. Rev. Lett.,2016

2. GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence;Abbott;Phys. Rev. Lett.,2016

3. GW170608: observation of a 19 solar-mass binary black hole coalescence;Abbott;Astrophys. J. Lett.,2017

4. GW170814: a three-detector observation of gravitational waves from a binary black hole coalescence;Abbott;Phys. Rev. Lett.,2017

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1. Black-hole formation in binary neutron star mergers: The impact of spin on the prompt-collapse scenario;Physical Review D;2024-06-06

2. Total r-process Yields of Milky Way Neutron Star Mergers;The Astrophysical Journal;2024-03-01

3. Measuring the Hubble Constant of Binary Neutron Star and Neutron Star–Black Hole Coalescences: Bright Sirens and Dark Sirens;The Astrophysical Journal Supplement Series;2024-01-22

4. Observational Prospects of Double Neutron Star Mergers and Their Multimessenger Afterglows: LIGO Discovery Power, Event Rates, and Diversity;The Astrophysical Journal;2023-07-26

5. The Central Engine of GRB170817A and the Energy Budget Issue: Kerr Black Hole versus Neutron Star in a Multi-Messenger Analysis;Universe;2023-06-08

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