| Authors |
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| Publication date |
2004
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| Journal |
Monthly Notices of the Royal Astronomical Society
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| Volume | Issue number |
354
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| Pages (from-to) |
L49-L53
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| Organisations |
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Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
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Faculty of Science (FNWI) - Informatics Institute (IVI)
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| Abstract |
We investigate the possibility that mass transfer early in the evolution of a massive binary can effect a reversal of the end states of the two components, resulting in a neutron star that forms before a black hole. In this sense, such systems would comprise the high-mass analogues of white dwarf-neutron star systems such as PSR B2303+46. One consequence of this reversal is that a second episode of mass transfer from the black hole progenitor star can recycle the nascent neutron star, extending the life of the pulsar.
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| Document type |
Article
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| Published at |
https://doi.org/10.1111/j.1365-2966.2004.08373.x
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| Published at |
http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004MNRAS.354L..49S&db_key=AST&high=41f4b95c5121568
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