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Soft gamma-ray repeaters and superstrong magnetic fields

โœ Scribed by T. Murakami


Publisher
John Wiley and Sons
Year
1999
Tongue
English
Weight
82 KB
Volume
320
Category
Article
ISSN
0004-6337

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โœฆ Synopsis


Four Soft Gamma-ray Repeaters were observed with ASCA, RXTE and BeppoSAX in X-ray. Two were already identified to a pulsar of 7.47 s and 5.16 s in period. The periods and the period derivatives enable us to estimate magnetic dipole moments. These are extremely strong of almost 10 15 Gauss. Shortage of the rotational energy to explain the observed luminosities and the SGR activities are naturally explained by the Magnetar model by Thompson and Duncun. A possibility to explain the classical GRBs by a giant energy release at the birth of magnetars is also mentioned.


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