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SN1987A: Temporal Models

Published online by Cambridge University Press:  13 May 2016

M. I. Wanas ,
M. Melek  and
M. E. Kahil
M. I. Wanas
Affiliation:
Astronomy Department, Faculty of Science, Cairo University, Giza, Egypt E-mail: wanas@mailer.scu.eun.eg
M. Melek
Affiliation:
Astronomy Department, Faculty of Science, Cairo University, Giza, Egypt E-mail: wanas@mailer.scu.eun.eg
M. E. Kahil
Affiliation:
Astronomy Department, Faculty of Science, Cairo University, Giza, Egypt E-mail: wanas@mailer.scu.eun.eg

Abstract

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We construct two temporal models for SN1987A. The first model assumes spin independent trajectories for massless particles, while the second assumes spin dependent ones. The suggested scheme can be applied to any supernova event.

Type
Supernovae, Pulsars, and the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 396 - 397
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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