Millisecond pulsars with extremely strong magnetic fields as a cosmological source of γ-ray bursts
- 11 June 1992
- journal article
- Published by Springer Nature in Nature
- Vol. 357 (6378) , 472-474
- https://doi.org/10.1038/357472a0
Abstract
No abstract availableKeywords
This publication has 26 references indexed in Scilit:
- Spatial distribution of γ-ray bursts observed by BATSENature, 1992
- The rotationally modulated Zeeman spectrum at nearly 10 to the 9th Gauss of the white dwarf PG 1031 + 234The Astrophysical Journal, 1987
- The period and magnetic field distributions of cataclysmic variables: Implications for their evolutionAstrophysics and Space Science, 1987
- Synchronization of magnetic stars in binary systemsThe Astrophysical Journal, 1983
- X-ray illumination of globular cluster puzzlesThe Astrophysical Journal, 1982
- Theory of pulsar magnetospheresReviews of Modern Physics, 1982
- Observed and derived parameters for 330 pulsarsThe Astronomical Journal, 1981
- On the nature of ?-ray burstsAstrophysics and Space Science, 1975
- On the Nature of Pulsars. I. TheoryThe Astrophysical Journal, 1969
- Rotating Neutron Stars, Pulsars and Supernova RemnantsNature, 1968