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Asymmetric Core-collapse of a Rapidly-rotating Massive Star

Published online by Cambridge University Press:  28 July 2017

Avishai Gilkis Open the ORCID record for Avishai Gilkis [Opens in a new window]
Avishai Gilkis*
Affiliation:
Department of Physics, Technion – Israel Institute of Technology, Haifa 3200003, Israel email: agilkis@technion.ac.il
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Abstract

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I 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.

Keywords

supernovae: generalstars: rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 400
Copyright
Copyright © International Astronomical Union 2017 

References

Couch, S. M. & O'Connor, E. P., 2014, ApJ, 785, 123 CrossRefGoogle Scholar
Fryxell, B., et al. 2000, ApJS, 131, 273 Google Scholar
Paxton, B., et al. 2011, ApJS, 192, 3 CrossRefGoogle Scholar
Spruit, H. C., 2002, A&A, 381, 923 Google Scholar