Published in
Oxford University Press, Monthly Notices of the Royal Astronomical Society, 2(474), p. 2419-2429, 2017
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 400
DOI: 10.1017/s1743921317003015
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Asymmetric core collapse of rapidly rotating massive star
Journal article published in 2017 by
Avishai Gilkis 
This paper is made freely available by the publisher.
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Abstract
AbstractI find high turbulent shearing in a neutron-rich accretion disk surrounding a proto-neutron star formed at the collapse of a rapidly-rotating MZAMS = 54M⊙ star. These might be features of superluminous supernovae powered by jets and/or magnetar spin-down.