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:
Runaway stars and pulsars near Crab Nebula, discussing binary system explosion and remnant motionread more
Citations
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Peculiar Objects in the Birthplaces of Radio Pulsars—Stellar-Mass Black Hole Candidates
Lisa Chmyreva,Gregory Beskin +1 more
Book ChapterDOI
Neutrino-Electron Interactions in External Active Media
TL;DR: In this paper, the neutrino-electron processes in external active media were investigated and the four-vector of the mean energy and momentum losses due to the process was derived.
Journal ArticleDOI
Millisecond Pulsar Velocities
Maurizio Toscano,Maurizio Toscano,J. S. Sandhu,Matthew Bailes,Richard N. Manchester,Richard N. Manchester,M. C. Britton,Shrinivas R. Kulkarni,S. B. Anderson,Ben Stappers +9 more
TL;DR: In this paper, the mean transverse velocity of 13 millisecond pulsars (MSPs) was found to be 85+/-13 km/s, a value consistent with most models for the origin and evolution of MSPs and approximately a factor of four lower than that of ordinary pulsars.
Journal ArticleDOI
Neutrino trigger of the magnetorotational mechanism of a natal-pulsar kick
A. V. Kuznetsov,N. V. Mikheev +1 more
TL;DR: In this paper, the neutrino effect on the plasma of the supernova-core envelope in a magnetorotational explosion accompanied by the generation of a strong toroidal magnetic field leads to a redistribution of the magnetic field B in the upper and lower hemispheres of a supernova core envelope.
Journal ArticleDOI
Relevance of variable negative radial velocities to models of sco x-1.
TL;DR: In this paper, it was shown that the emission line radial velocities of Sco X-1 are variable on a time scale of days or even hours, with an amplitude of perhaps ±50 km s−1, or occasionally somewhat greater.