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High Energy γ-ray Observations of SN 1987A

Published online by Cambridge University Press:  25 April 2016

R.K. Sood ,
J.A. Thomas ,
L. Waldron ,
R.K. Manchanda ,
G.K. Rochester ,
T.J. Sumner ,
G. Frye ,
T. Jenkins ,
R. Koga  and
P. Ubertini
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R.K. Sood
Affiliation:
Australian Defence Force Academy, Canberra
J.A. Thomas
Affiliation:
Australian Defence Force Academy, Canberra
L. Waldron
Affiliation:
Australian Defence Force Academy, Canberra
R.K. Manchanda
Affiliation:
Australian Defence Force Academy, Canberra
G.K. Rochester
Affiliation:
Imperial College of Science, Technology & Medicine, London
T.J. Sumner
Affiliation:
Imperial College of Science, Technology & Medicine, London
G. Frye
Affiliation:
Case Western Reserve University, Cleveland, USA
T. Jenkins
Affiliation:
Case Western Reserve University, Cleveland, USA
R. Koga
Affiliation:
Case Western Reserve University, Cleveland, USA
P. Ubertini
Affiliation:
Istituto di Astroflsica Spaziale, Frascati, Italy
A. Bazzano
Affiliation:
Istituto di Astroflsica Spaziale, Frascati, Italy
C. La Padula
Affiliation:
Istituto di Astroflsica Spaziale, Frascati, Italy
R. Staubert
Affiliation:
Astronomisches Institut der Universität Tübingen, West Germany
E. Kendziorra
Affiliation:
Astronomisches Institut der Universität Tübingen, West Germany
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Abstract

SN 1987A has been observed with a combined high energy γ-ray (50-500 MeV) and hard X-ray (15-150 keV) payload during a balloon flight on 5 April 1988 from Alice Springs, Australia. The γ-ray observations, along with our earlier ones on 19 April 1987 are the only such observations of the supernova to date. The γ-ray detector characteristics are described. The preliminary results of the recent flight and their implications in terms of the known supernova parameters are discussed.

Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 7 , Issue 4 , 1988 , pp. 486 - 489
Copyright
Copyright © Astronomical Society of Australia 1988

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