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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On the formation of compact, massive subsystems in stellar clusters and its relation with intermediate-mass black holes
TL;DR: In this paper, the early formation phase of a dense, massive sub-system (MSS) in several GCs models using a recently developed semi-analytical treatment of the mass segregation process was studied.
Journal ArticleDOI
Resonant spin-flavor precession of neutrinos and pulsar velocities
TL;DR: In this article, a new mechanism for the generation of large velocities based on an asymmetric emission of neutrinos during the supernova explosion is proposed, which involves the resonant spin-flavor precession of neutrons with a transition magnetic moment in the magnetic field of a supernova.
Journal ArticleDOI
Pulsar kicks induced by spin flavour oscillations of neutrinos in gravitational fields
TL;DR: In this article, the origin of pulsar kicks is reviewed in the framework of the spin-flip conversion of neutrinos propagating in the gravitational field of a magnetized protoneutron star.
Journal ArticleDOI
Pulsar kicks by anisotropic neutrino emission from quark matter in strong magnetic fields
TL;DR: In this paper, a pulsar acceleration mechanism based on asymmetric neutrino emission from the direct quark Urca process in the interior of proto neutron stars is discussed, where the neutrinos are emitted by the cooling strange quark matter core with an anisotropic caused by a strong magnetic field.
Journal ArticleDOI
Populating the Galaxy with pulsars - II. Galactic dynamics
Paul D. Kiel,Jarrod R. Hurley +1 more
TL;DR: In this paper, a complete pulsar population synthesis code that accounts for isolated and binary pulsar evolution, Galactic spatial evolution and pulsar survey selection effects is presented, along with the second component which focuses on following the orbits of the pulsars within the Galactic potential.