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On the Origin of Kepler's Supernova Remnant

Published online by Cambridge University Press:  04 August 2017

R. Bandiera
R. Bandiera*
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy

Extract

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Aim of my poster is to show that Kepler's supernova progenitor was a massive star, rather than an old population object, as commonly accepted. The star was subject to strong mass loss, and the present remnant is due to the interaction of the blast wave with dense circumstellar matter

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 127
Copyright
Copyright © Reidel 1987