Results 101 to 110 of about 17,664 (256)
Orbital spin dynamics of a millisecond pulsar around a massive BH with a general mass quadrupole [PDF]
, 2020 Tom Kimpson, Kinwah Wu, Silvia Zane
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Are millisecond pulsars different than “Normal” pulsars? [PDF]
International Astronomical Union Colloquium, 1992 AbstractWhile millisecond pulsars have very different period parameters and a different evolutionary history compared to “normal” pulsars, the properties of their pulsed emission are remarkably similar to those of normal pulsars.
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The Astrophysical JournalWe use cyclic spectroscopy to perform high-frequency resolution analyses of multihour baseband Arecibo observations of the millisecond pulsar PSR B1937+21.
Jacob E. Turner +10 more
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New millisecond pulsars in globular clusters
AIP Conference Proceedings, 2001 Paper presented at the 20th Texas Symposium on Relativistic Astrophysics, 10-15 December 2000 - Austin ...
D'AMICO, NICOLO' +5 more
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COBIPULSE: A Systematic Search for Compact Binary Millisecond Pulsars
The Astrophysical JournalWe report here the results obtained from a systematic optical photometric survey aimed at finding new compact binary millisecond pulsars (also known as “spiders”): the COmpact BInary PULsar SEarch. We acquired multiband optical images over 1 yr around 33
Marco Turchetta +7 more
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GRAVITATIONAL RADIATION FROM ACCRETING MILLISECOND PULSARS
The Eleventh Marcel Grossmann Meeting, 2008 It is widely assumed that the observed reduction of the magnetic field of millisecond pulsars can be connected to the accretion phase during which the pulsar is spun up by mass accretion from a companion. A wide variety of reduction mechanisms have been proposed, including the burial of the field by a magnetic mountain, formed when the accreted matter ...
Vigelius, Matthias +2 more
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The Spectrum of the Millisecond Pulsar J0218+4232 - Theoretical Interpretations [PDF]
, 2002 J. Dyks, B. Rudak
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Discovery of Four Isolated Millisecond Pulsars
The Astrophysical Journal, 1997 We report the discovery of four isolated millisecond pulsars found as part of the Parkes 436 MHz survey of the southern sky. Three of the pulsars, PSRs J1024-0719, J1744-1134, and J2124-3358, are close to the Sun (d <360 pc) and have very low luminosities, ≲0.5 mJy kpc2. The other, PSR J0711-6830, is of intermediate luminosity.
Bailes, M. +9 more
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