The binary evolution of SAX J1808.4−3658: implications of an evolved donor star
Author:
Affiliation:
1. School of Physics and Astronomy, Monash University, Clayton, Victoria 3800, Australia
2. National Research Council of Canada, Herzberg Astronomy and Astrophysics Research Centre, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada
Abstract
Funder
National Research Council Canada
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staa1234/33175258/staa1234.pdf
Reference51 articles.
1. An alternative to common envelope evolution
2. A Brown Dwarf Companion for the Accreting Millisecond Pulsar SAX J1808.4−3658
3. A NICER Thermonuclear Burst from the Millisecond X-Ray Pulsar SAX J1808.4–3658
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1. The Impact of Angular Momentum Loss on the Outcomes of Binary Mass Transfer;The Astrophysical Journal;2023-11-20
2. The Effect of Irradiation on the Spin of Millisecond Pulsars;The Astrophysical Journal Letters;2023-10-01
3. A New Flaring Black Widow Candidate and Demographics of Black Widow Millisecond Pulsars in the Galactic Field;The Astrophysical Journal;2022-12-01
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