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N49: The Site of a Gamma-ray Burst. Preliminary Results from X-ray Observations

Published online by Cambridge University Press:  04 August 2017

G. Pizzichini ,
T. L. Cline ,
U. D. Desai ,
B. J. Teegarden ,
W. D. Evans ,
E. E. Fenimore ,
R. W. Klebesadel ,
J. G. Laros ,
K. Hurley  and
M. Niel
...Show all authors
G. Pizzichini
Affiliation:
Istituto TESRE/CNR, Bologna
T. L. Cline
Affiliation:
NASA/GSFC, Greenbelt
U. D. Desai
Affiliation:
NASA/GSFC, Greenbelt
B. J. Teegarden
Affiliation:
NASA/GSFC, Greenbelt
W. D. Evans
Affiliation:
LASL, Los Alamos
E. E. Fenimore
Affiliation:
LASL, Los Alamos
R. W. Klebesadel
Affiliation:
LASL, Los Alamos
J. G. Laros
Affiliation:
LASL, Los Alamos
K. Hurley
Affiliation:
CESR (CNRS/UPS), Toulouse
M. Niel
Affiliation:
CESR (CNRS/UPS), Toulouse
G. Vedrenne
Affiliation:
CESR (CNRS/UPS), Toulouse

Abstract

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The error box of the unusual Gamma-Ray Burst of March 5, 1979 falls completely inside the optical and radio image of the Supernova Remnant N49 in the Large Magellanic Cloud. This region was observed twice in x-rays with the High Resolution Imager of the Einstein Observatory, six weeks and nearly two years after the Gamma-Ray Burst. We show the comparison between the two observations.

Type
VI. Supernova Remnants in Other Galaxies
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 573 - 577
Copyright
Copyright © Reidel 1983 

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