Results 101 to 110 of about 6,438 (185)
Gravitational Redshift for Rapidly Rotating Neutron Stars
The oblate Schwarzschild (OS) approximation is a method often used to compute the flux of X-rays emitted from a rapidly rotating neutron star. In this approximation, the oblate shape of the rotating star is embedded in the Schwarzschild metric, which is ...
Zsombor Jakab, Sharon M. Morsink
doaj +1 more source
We compare the observational properties of rotation-powered binary millisecond pulsars (BMSPs) in the Galactic Field with various companion types. First, BMSPs with diverse companion types exhibit different properties in the relation of binary orbital ...
De-Hua Wang +2 more
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A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437–4715
We report Bayesian inference of the mass, radius, and hot X-ray emitting region properties—using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest rotation-powered millisecond X-ray pulsar, PSR J0437−4715. Our modeling is
Devarshi Choudhury +19 more
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Thermal X-ray emission from rotation-powered millisecond pulsars, shaped by gravitational lensing and the beaming of the surface radiation, provides critical insights into neutron star properties. This approach has been the focus of observations with the
Tong Zhao +2 more
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Investigation of Accuracy of TOA and SNR of Radio Pulsar Signals for Vehicles Navigation. [PDF]
Kabakchiev H +4 more
europepmc +1 more source
The Timing Evolution of the Magnetar Swift J1818.0–1607 during a Period of Reduced Activity
We report results from an observational campaign of the radio-loud magnetar Swift J1818.0−1607 using the Green Bank Telescope at 2.0 GHz that began in 2021 November, during a period of reduced activity approximately 20 months after its 2020 March ...
Moaz Abdelmaguid +5 more
doaj +1 more source
Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]
Caleb M +21 more
europepmc +1 more source
Through a detailed timing analysis of Fermi-LAT data, the rotational behavior of the γ -ray pulsar PSR J1522−5735 was tracked from 2008 August (MJD 54692) to 2024 January (MJD 60320).
S. Q. Zhou +7 more
doaj +1 more source
A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism. [PDF]
Zhu W +36 more
europepmc +1 more source

