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Dany Page: Instituto de Astronomia, UNAM (National Autonomous University of Mexico)
Do Supernovae Make or Kill Pulsars?
I'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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Slavko Bogdanov: Columbia
X-rays from Radio Millisecond Pulsars
