Results 81 to 90 of about 16,242 (188)
Spider pulsars represent a unique subclass of radio millisecond pulsars in binaries, and are further categorized into black widows and redbacks according to the mass of the low-mass companion.
Chunyan Lu +5 more
doaj +1 more source
Investigation of Accuracy of TOA and SNR of Radio Pulsar Signals for Vehicles Navigation. [PDF]
Kabakchiev H +4 more
europepmc +1 more source
Discovery of the Accretion-powered Millisecond X-Ray Pulsar IGR J00291+5934 [PDF]
D. K. Galloway +4 more
openalex +1 more source
SAX J1808.4−3658, an accreting millisecond pulsar shining in gamma rays? [PDF]
E. de Oña Wilhelmi +9 more
openalex +1 more source
Pulse profile stability in millisecond pulsars (MSPs) is a key factor in achieving high-precision timing essential for detecting nanohertz gravitational waves with pulsar timing arrays (PTAs).
Ankita Ghosh +5 more
doaj +1 more source
Chandra observations of the millisecond X-ray pulsar IGR J00291+5934 in quiescence [PDF]
P. G. Jonker +7 more
openalex +1 more source
Pulse Profile Variability of PSR J1022+1001 in NANOGrav Data
Pulse profile stability is a central assumption of standard pulsar timing methods. Thus, it is important for pulsar timing array experiments such as the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) to account for any pulse ...
William Fiore +48 more
doaj +1 more source
Signal of Quark Deconfinement in Millisecond Pulsars and Reconfinement\n in Accreting X-ray Neutron Stars [PDF]
Norman K. Glendenning, Fridolin Weber
openalex +1 more source
Orbital spin dynamics of a millisecond pulsar around a massive BH with a general mass quadrupole [PDF]
Tom Kimpson, Kinwah Wu, Silvia Zane
openalex +1 more source
The millisecond pulsar J1713+0747 underwent a sudden and significant pulse shape change between 2021 April 16 and 17 (MJDs 59320 and 59321). Subsequently, the pulse shape gradually recovered over the course of several months.
Ross J. Jennings +43 more
doaj +1 more source

