Results 141 to 150 of about 16,963 (231)
Formation of binary millisecond pulsars by accretion-induced collapse of white dwarfs [PDF]
Jarrod R. Hurley +4 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
doaj +1 more source
No low-frequency turn-over in the spectra of millisecond pulsars [PDF]
A. D. Kuzmin, B. Ya. Losovsky
openalex +1 more source
FAST Discovery of Eight Isolated Millisecond Pulsars in NGC 6517
We present the discovery of eight isolated millisecond pulsars in globular cluster (GC) NGC 6517 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST).
Dejiang Yin +16 more
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Born to be recycled: a comprehensive population synthesis of the Galactic millisecond pulsars [PDF]
Mattéo Sautron +4 more
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Eccentric Binary Millisecond Pulsars
In this paper we review the recent discovery of several millisecond pulsars (MSPs) in eccentric binary systems. Timing these MSPs we were able to estimate (and in one case precisely measure) their masses. These results suggest that, as a class, MSPs have a much wider range of masses (1.3 to > 2 solar masses) than the normal and mildly recycled ...
openaire +2 more sources
We employed the fast-folding algorithm on L -band globular cluster (GC) observations taken with the Five-hundred-meter Aperture Spherical radio Telescope to search for new pulsars, especially those with a long rotational period.
Yaowei Li +17 more
doaj +1 more source
Burst-recurrence properties revealed with Insight-HXMT and NICER for the newly discovered accreting millisecond pulsar MAXI J1816–195 [PDF]
Peng-Ju Wang +14 more
openalex +1 more source
Modulated gamma-ray emission from compact millisecond pulsar binary systems [PDF]
W. Bednarek
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Eclipsing Millisecond Pulsars with He Star Companions
Eclipsing millisecond pulsars (MSPs) are a type of pulsar binaries with close orbits (≲1.0 day). They are important objects for studying the accretion history of neutron stars (NSs), pulsar winds, and the origin of isolated MSPs, etc.
Yunlang Guo +4 more
doaj +1 more source

