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Title: Study of the precision of the gamma-ray burst source locations obtained with the Ulysses/PVO/CGRO network

Conference · · AIP Conference Proceedings (American Institute of Physics); (United States)
OSTI ID:7025326
 [1];  [2];  [3]; ;  [4]; ; ; ; ;  [5]; ;  [6]
  1. NASA/Goddard Space Flight Center, Code 661, Greenbelt, Maryland 20771 (United States)
  2. University of California, Space Sciences Laboratory, Berkeley, California 94720 (United States)
  3. Max-Planck Institut fuer Extraterrestrische Physik, D8046 Garching (Germany)
  4. Centre d'Etude Spatiale des Rayonnements, Toulouse (France)
  5. NASA/Marshall Space Flight Center, ES-62, Huntsville, Alabama 35812 (United States)
  6. Los Alamos National Laboratory, MS D436, Los Alamos, New Mexico 87545 (United States)

The interplanetary gamma-ray burst network of the [ital Ulysses], [ital Compton]-[ital GRO], and [ital Pioneer]-[ital Venus] [ital Orbiter] missions has made source localizations with fractional-arc-minute precision for a number of events, and with auxiliary data, will provide useful annular-segment loci for many more. These studies have, thus far, yielded one possible counterpart, a [ital Rosat] x-ray association with the 92 May 1 burst. Similar to the historic 1978 November 19 burst/[ital Einstein] association, this possibility gives hope that network studies will provide a fundamental source clue for classical' bursts, just as a second supernova remnant in a network-defined source field has done for sgr events.

OSTI ID:
7025326
Report Number(s):
CONF-9310252-; CODEN: APCPCS
Journal Information:
AIP Conference Proceedings (American Institute of Physics); (United States), Vol. 307:1; Conference: 2. gamma-ray burst workshop, Huntsville, AL (United States), 20-22 Oct 1993; ISSN 0094-243X
Country of Publication:
United States
Language:
English

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