Precise source location of the anomalous 1979 March 5 gamma-ray transient | Zendy

T. L. Cline | Zendy; U. D. Desai | Zendy; B. J. Teegarden | Zendy; W. D. Evans | Zendy; R. W. Klebesadel | Zendy; J. G. Laros | Zendy; C. Barat | Zendy; Kevin Hurley | Zendy; M. Niel | Zendy; G. Védrenne | Zendy

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Precise source location of the anomalous 1979 March 5 gamma-ray transient

Author(s) -

T. L. Cline,

U. D. Desai,

B. J. Teegarden,

W. D. Evans,

R. W. Klebesadel,

J. G. Laros,

C. Barat,

Kevin Hurley,

M. Niel,

G. Védrenne

Publication year - 1982

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/183766

Subject(s) - physics , gamma ray , transient (computer programming) , astrophysics , x ray transient , astronomy , neutron star , computer science , operating system

Refinements in the source direction analysis of the observations of the unusual 1979 March 5 gamma-ray transient are presented. The final results from the interplantary gamma-ray burst network produce a 0.1 arcmin/sup 2/ error box. It is nested inside the initially determined 2 arcmin/sup 2/ source region of Evans et al. that identified the supernova remnant N49 in the Large Magellanic Cloud as a possible source. This smaller source location is within both the optical and X-ray contours of N49 although not positioned at either contour center.

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