Changes between Version 3 and Version 4 of Talks/Falll2011/SpecialSeminars/111110a


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Timestamp:
11/07/11 18:26:02 (15 years ago)
Author:
jules@…
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  • Talks/Falll2011/SpecialSeminars/111110a

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    55I'll present results of numerical simulations of post-supernova hypercritical (i.e. highly super-Eddington) accretion onto a new-born magnetized neutron star. The purpose of these is to study whether such accretion is able to submerge the magnetic field and produce a non-magnetized star. CCOs may be candidates for such demagnetized neutron stars.
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    99Slavko Bogdanov (Columbia)