Results 61 to 70 of about 3,309 (210)
White Noises on Different Stokes Components of Six Millisecond Pulsars
The Astrophysical JournalWe presented measurements of jitter noise and radiometer noise for the Stokes parameters I , L , and V in six millisecond pulsars from the International Pulsar Timing Array sample, based on FAST observations.
S. N. Sun, N. Wang, W. M. Yan
doaj +1 more source
Multi-wavelength study of binary millisecond pulsars [PDF]
, 2021 The main object of my research activity has been the multi-wavelength study of the temporal evolution of binary millisecond pulsars (MSPs), from the accretion phase to the radio pulsar state.
MIRAVAL ZANON ARIANNA
core
Population synthesis of millisecond and submillisecond pulsars
, 1998 Known millisecond pulsars have periods longer than 1.558 ms. Recycled in binary systems, neutron stars can attain very short spin periods. In this Letter, we investigate the expected properties of the millisecond pulsar distribution by simulating ...
D'AMICO, NICOLO' +3 more
core +1 more source
The Relationships between Emission Geometry and Jitter Noise in Millisecond Pulsars
The Astrophysical JournalThe relationships between several parameters of an emission geometry and jitter noise in 17 millisecond pulsars (MSPs) are investigated. By assuming the jitter noise is due only to a pulse variation in phase, the former can be modeled as changes in the ...
R. Yuen
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Searching for sub-millisecond pulsars: A theoretical view
, 2007 Sub-millisecond pulsars should be triaxial (Jacobi ellipsoids), which may not spin down to super-millisecond periods via gravitation wave radiation during their lifetimes if they are extremely low mass bare strange quark stars.
Xu, Renxin +3 more
core +1 more source
Evidence for a Minimum Ellipticity in Millisecond Pulsars [PDF]
The Astrophysical Journal Letters, 2018 Abstract Neutron stars spin down over time due to a number of energy-loss processes. We provide tantalizing population-based evidence that millisecond pulsars (MSPs) have a minimum ellipticity of ϵ ≈ 10−9 around their spin axis and that, consequently, some spin down mostly through gravitational-wave emission.
G. Woan +4 more
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Polarimetry of millisecond pulsars
The Astrophysical Journal, 1990 The mean polarization profiles of several fast pulsars were measured. Observations of pulsar PSR 1937 + 21 are similar to previously published results, except that a shallower position angle was found to swing across the pulse at low frequency; for the first time, the occurrence of orthogonal mode switching at all frequencies is explicitly demonstrated.
Stephen E. Thorsett +1 more
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Observations of Nine Millisecond Pulsars at 8600 MHz Using the TMRT
The Astrophysical JournalWe report detection results of nine millisecond pulsars (MSPs) at 8600 MHz using simultaneous 2250 and 8600 MHz observations conducted with the Shanghai Tian Ma Radio Telescope.
Xiao-Wei Wang +9 more
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Probing neutron star physics using accreting neutron stars
EPJ Web of Conferences, 2010 We give an obervational overview of the accreting neutron stars systems as probes of neutron star physics. In particular we focus on the results obtained from the periodic timing of accreting millisecond X-ray pulsars in outburst and from the ...
Patruno A.
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A millisecond pulsar in a stellar triple system [PDF]
Nature, 2014 17 pages, 3 figures, 1 table. Published online by Nature on 5 Jan 2014.
Ransom, S.M. +20 more
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