(Q59092798)

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Millisecond pulsars with extremely strong magnetic fields as a cosmological source of γ-ray bursts

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Millisecond pulsars with extremely strong magnetic fields as a cosmological source of γ-ray bursts (English)

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V. V. Uso

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1

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English

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June 1992

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357

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6378

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472–474

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https://scigraph.springernature.com/pub.10.1038/357472a0

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Spatial distribution of γ-ray bursts observed by BATSE

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The period and magnetic field distributions of cataclysmic variables : implications for their evolution

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The rotationally modulated Zeeman spectrum at nearly 10 to the 9th Gauss of the white dwarf PG 1031 + 234

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X-ray illumination of globular cluster puzzles

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Observed and derived parameters for 330 pulsars

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Synchronization of magnetic stars in binary systems

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Rotating Neutron Stars, Pulsars and Supernova Remnants

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On the nature of pulsars. I. Theory

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Theory of pulsars: polar gaps, sparks, and coherent microwave radiation

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On Gauge Invariance and Vacuum Polarization

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Photon splitting and photon dispersion in a strong magnetic field

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Gam-quanta capture by magnetic field and pair creation suppression inpulsars

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Gamma-ray bursters at cosmological distances

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Are gamma-ray bursts optically thick?

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The appearance of cosmic fireballs

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Generation of gamma-bursts by old magnetic neutron stars

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Statistics of cosmological gamma-ray bursts

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1048532393

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(Q59092798)

Millisecond pulsars with extremely strong magnetic fields as a cosmological source of γ-ray bursts

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