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9 - Types for the galactic supernovae

Published online by Cambridge University Press:  11 August 2009

B. E. Schaefer
Affiliation:
Louisiana State University, Baton Rouge Louisiana 70803 USA
Peter Höflich
Affiliation:
University of Texas, Austin
Pawan Kumar
Affiliation:
University of Texas, Austin
J. Craig Wheeler
Affiliation:
University of Texas, Austin
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Summary

Abstract

The six galactic supernovae within the last millennium are critical to all work on the relationships between supernovae and their remnants. Yet this field has been dogged by controversy and discarded arguments. Even during the Wheeler Symposium, we had successive speakers give different type assignments to individual events. In an effort to at least define the confusion, I have polled a group of leading experts as to their current thinking on the types for each of the historical events. This complements a similar poll made a decade ago. We must realize that these results are not voting-on-the-truth, but is rather an expression of community opinion. The recent poll has the following results. SN1006 is universally agreed to be a Type Ia event. SN1054 (the Crab) is puzzling in many ways, but it must be from some sort of a core collapse event. SN1181 is thought to be a core collapse event primarily on the basis of its remnant being a plerion like the Crab. SN1572 (Tycho's) is agreed to be a Type Ia event. SN1604 (Kepler's) has no consensus, with all types being claimed and denied. Cas A is unanimously agreed to not be a Type Ia event, but after that all possibilities find their champions.

The polls

The six galactic supernovae within the last millennium (SN1006, SN1054, SN1181, SN1572, SN1604, and Cas A) all have very well observed remnants. A key question for understanding these remnants is the type of the original explosion.

Type
Chapter
Information
Cosmic Explosions in Three Dimensions
Asymmetries in Supernovae and Gamma-Ray Bursts
, pp. 81 - 84
Publisher: Cambridge University Press
Print publication year: 2004

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References

Bandiera, R. 1987. Astrophys. J., 319, 885CrossRef
Hill, L. C. 1993. QJRAS, 34, 73
Raymond, J. C. 1984. ARA&A, 22, 75CrossRef
Schaefer, B. E. 1996a. Astrophys. J., 459, 438CrossRef
Schaefer, B. E. 1996b. Astrophys. J., 464, 404CrossRef
Bergh, S. 1988. Astrophys. J., 327, 156CrossRef
Bergh, S. 1994. Astrophys. J., 425, 208
Weiler, K. W. & Sramek, R. A. 1988. ARA&A, 26, 247

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