Changes between Version 3 and Version 4 of Talks/Falll2011/SpecialSeminars/111110a
- Timestamp:
- 11/07/11 18:26:02 (15 years ago)
Legend:
- Unmodified
- Added
- Removed
- Modified
-
Talks/Falll2011/SpecialSeminars/111110a
v3 v4 5 5 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. 6 6 7 ============================================================================================================================= ========7 ============================================================================================================================= 8 8 9 9 Slavko Bogdanov (Columbia)
