Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...207...55v&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 207, no. 1, Dec. 1988, p. 55-69.
Astronomy and Astrophysics
Astrophysics
17
Astronomical Models, Gamma Ray Bursts, Neutron Stars, Stellar Flares, Binary Stars, Cataclysmic Variables, Light Curve, Magnetic Field Reconnection, Magnetic Stars, Solar X-Rays
Scientific paper
The authors establish a similarity between the gamma ray burst characteristics and solar hard X-ray flares. They show that all the temporal and spectral features observed in gamma ray bursts are also seen in solar hard X-ray flares. The only distinction is in the energy contents of the two. The authors suggest that the gamma-ray bursts originate from sources which have Sun like activity. Large scale Sun like activity has been observed in flare stars, RS CVn binaries and cataclysmic variables which are grouped together as the magnetically active stellar systems. The energetics of such systems is discussed and it is shown that these systems have enough energy to produce gamma-ray bursts. The authors then attempt positional identification between gamma-ray burst error boxes and the magnetically active stellar systems and find an association of 34 objects.
Rao Ravi A.
Vahia Mayank N.
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