An outburst of relativistic particles from the soft γ-ray repeater SGR1900+14-Reference-Cited by-同舟云学术

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An outburst of relativistic particles from the soft γ-ray repeater SGR1900+14

Published:1999-03 Issue:6723 Volume:398 Page:127-129
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Frail D. A.,Kulkarni S. R.,Bloom J. S.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/18163.pdf

Reference23 articles.

1. Kulkarni, S. R. & Frail, D. A. Identification of a supernova-remnant coincident with the soft γ-ray repeater SGR1806−20. Nature 365, 33–35 (1993).

2. Thompson, C. & Duncan, R. C. The soft gamma repeaters as very strongly magnetized neutron stars—I. Radiative mechanism for outbursts. Mon. Not. R. Astron. Soc. 275, 255–300 (1995).

3. Thompson, C. & Duncan, R. C. The soft gamma repeaters as very strongly magnetized neutron stars. II. Quiescent neutrino, X-ray, and Alven wave emission. Astrophys. J. 473, 322–342 (1996).

4. Mazets, E. P., Golenetskii, S. V., Il'inskii, V. N., Aptekar', R. L. & Gur'yan, Yu. A. Observations of a flaring X-ray pulsar in Dorado. Nature 282, 587–589 (1979).

5. Kouveliotou, C. et al. An X-ray pulsar with a super-strong magnetic field in the soft γ-ray repeater SGR1806−20. Nature 393, 235–237 (1998).

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