Search results for "Spin-up"

showing 3 items of 3 documents

The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars

2020

arXiv:2012.01346v1

Astrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsMagnetarQuantitative Biology::OtherComputer Science::Digital Libraries01 natural sciencesNeutron starsX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesMagnetarsAccretion disks magnetars neutron stars pulsar X-rays:binaries X-rays:burstseducationX-rays: bursts010303 astronomy & astrophysicsPulsarsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_study010308 nuclear & particles physicsCrab PulsarAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsAccretion (astrophysics)Neutron starSpace and Planetary ScienceAccretion disksSpin-upAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Spin-up instability of electromagnetically levitated spherical bodies

2000

Stability of a solid sphere in both uniform and linear alternating magnetic fields is considered with respect to virtual rotations. When the frequency of the alternating magnetic field exceeds a certain critical threshold depending on the configuration of the field, the sphere is found to spin up around a horizontal axis. The physical mechanism of this instability is the same as that of operation of a single-phase induction motor. Sufficiently small rotational disturbances can be completely suppressed by imposing an axial steady magnetic field of strength comparable to that of the alternating field. Nonlinear stability analysis shows that for sufficiently high frequencies, spin-up can be ca…

PhysicsClassical mechanicsField (physics)Electromagnetic suspensionMechanicsElectrical and Electronic EngineeringSpin-upElectrical conductorInstabilityInduction motorMagnetic levitationElectronic Optical and Magnetic MaterialsMagnetic fieldIEEE Transactions on Magnetics
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Discovery of a Transition to Global Spin-up in EXO 2030+375

2005

EXO 2030+375, a 42-second transient X-ray pulsar with a Be star companion, has been observed to undergo an outburst at nearly every periastron passage for the last 13.5 years. From 1994 through 2002, the global trend in the pulsar spin frequency was spin-down. Using RXTE data from 2003 September, we have observed a transition to global spin-up in EXO 2030+375. Although the spin frequency observations are sparse, the relative spin-up between 2002 June and 2003 September observations, along with an overall brightening of the outbursts since mid 2002 observed with the RXTE ASM, accompanied by an increase in density of the Be disk, indicated by infrared magnitudes, suggest that the pattern obse…

PhysicsOscillationBe starInfraredAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsPulsarSpace and Planetary SciencePrecessionCondensed Matter::Strongly Correlated ElectronsAstrophysics::Earth and Planetary AstrophysicsSpin-upSpin-½The Astrophysical Journal
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