Results 91 to 100 of about 3,309 (210)
Population synthesis of wide binary millisecond pulsars
Four evolutionary channels leading to the formation of wide binary millisecond pulsars are investigated. The majority of binary millisecond pulsars are found to descend from systems in which the most massive component undergoes a common-envelope phase ...
Kolb, U., Willems, B.
core +1 more source
Millisecond Pulsar Surveys [PDF]
In 1982 a new class of pulsars was defined by the discovery of a star with a millisecond rotation period, 1.6 ms. In the past 3.5 years two additional pulsars with millisecond periods have been discovered. The rapid spin of these pulsars is attributed to mass transfer in a low-mass binary progenitor system.
openaire +1 more source
Kinematics of low-mass X-ray binaries and millisecond pulsars
The kinematic properties of low-mass X-ray binaries and millisecond pulsars have been studied with the help of a Monte Carlo simulation. It is found that the kinematic properties of these two populations are consistent with each other, which supports the
Ramachandran, R., Bhattacharya, D.
core +1 more source
Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey
We present phase-connected timing ephemerides, polarization pulse profiles, and Faraday rotation measurements of 12 pulsars discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio Astronomy FAST Survey.
D. Zhao +42 more
doaj +1 more source
Polarimetric profiles of 27 millisecond pulsars
We present high time resolution polarimetric profiles of 27 predominantly southern hemisphere millisecond pulsars, 15 of which have no previously published polarimetry.
van Straten, W (15510356) +3 more
core
On the Number of Confirmed Pulsar Planets: The Rule of Six
Since the first definitive exoplanet detection, the three planets around millisecond radio pulsar PSR B1257+12, few more pulsar planets (PPs) have been reported.
Silas G. T. Laycock +1 more
doaj +1 more source
A Survey for Millisecond Pulsars
We have searched 960 square degrees of sky for radio pulsars, using the 305 m telescope at Arecibo, Puerto Rico. The 430 MHz survey reached a limiting sensitivity for slow pulsars of 0.7 mJy using a dual-polarization, 32 channel filterbank over 8 MHz of ...
S. R. Kulkarni +6 more
core
Three binary millisecond pulsars in NGC 6266
We present rotational and astrometric parameters of three millisecond pulsars located near the center of the globular cluster NGC 6266 (M62), resulting from timing observations with the Parkes radio telescope.
Manchester RN +6 more
core +1 more source
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

