Journal ArticleDOI
Runaway stars and the pulsars near the crab nebula.
TLDR
Runaway stars and pulsars near Crab Nebula, discussing binary system explosion and remnant motion as discussed by the authors, discussing binary systems explosion and residual motion in the Crab Nebula and its surrounding area.Abstract:
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Journal ArticleDOI
Observations of Pulsar Spectra
TL;DR: In this paper, the spectral features in CP 0328, CP 0834, CP 1133, and CP 1919 were observed to drift systematically at rates compatible with a simple interstellar scintillation model.
Journal ArticleDOI
Separated at Birth: The Origin of the Pulsars B2020+28 and B2021+51 in the Cygnus Superbubble
TL;DR: In this paper, high-precision astrometric data have enabled the discovery of a pulsar pair (B2020+28 and B2021+51) that has a common origin in the Cygnus superbubble or in one of its related OB associations at an epoch that is comparable to the spin-down ages of the pulsars.
Journal ArticleDOI
Soft gamma-ray bursts from accreting compact objects
TL;DR: In this paper, the authors consider the possibility that the γ-ray bursts may originate from fleeting episodes of accretion onto compact galactic objects and discuss a particular example which appears promising, namely the triggering of bursts by solar-type flares in a binary companion.
Journal ArticleDOI
Neutrino oscillation mechanism for pulsar kicks reexamined
TL;DR: In this article, a general expression for the momentum asymmetry in terms of the neutrino energy flux gradient was derived, and it was shown that a nonvanishing effect is induced at the lowest order by a deformed neutrinosphere.
Journal ArticleDOI
Toward an Empirical Theory of Pulsar Emission. XI. Understanding the Orientations of Pulsar Radiation and Supernova “Kicks”
TL;DR: The rotational orientation of most pulsars can be inferred only from the (fiducial) polarization angle of their radiation, when their beam points directly at the Earth and the emitting polar fluxtube field is k to the rotation axis as discussed by the authors.