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Historical Novæ and Supernovæ

Published online by Cambridge University Press:  03 March 2020

A. Pagnotta ,
D. W. Hamacher ,
K. Tanabe ,
V. Trimble  and
N. Vogt
A. Pagnotta
Affiliation:
Department of Physics and Astronomy, College of Charleston, SC 29424, USA email: pagnotta@cofc.edu
D. W. Hamacher
Affiliation:
Department of Indigenous Studies, Macquarie University, NSW 2109, Australia
K. Tanabe
Affiliation:
Okayama University of Science, Okayama, Japan
V. Trimble
Affiliation:
Department of Physics and Astronomy, University of California, Irvine, CA 92697-4575, USA
N. Vogt
Affiliation:
Instituto de Física y Astronomía, Universidad de Valparaíso, Valparaíso, Chile
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Abstract

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This paper brings together the chief points raised during FM5 by astronomers, archaeologists, and historians whose research interests centred on novæ and supernovæ. The common focus was the use of historical observations to study transient astronomical phenomena. The presenters covered a wide variety of topics within that theme, and this report summarizes some of the aspects specific to historical novæ and supernovæ.

Keywords

(stars:) novaecataclysmic variables(stars:) supernovae: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 171 - 175
Copyright
© International Astronomical Union 2020

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