Results 71 to 80 of about 512 (177)

Formation and nature of “Huntsman” binary pulsars

open access: yesAstronomy & Astrophysics
Context. “Spider” systems are a class of close binaries in which a neutron star first accretes from a normal companion, and later ablates it in some cases. New observations have expanded this category, with the addition of a “Huntsman” group, tentatively linked to a short donor phase along the red bump along the secondary evolutionary track. Aims.
O. G. Benvenuto   +6 more
openaire   +2 more sources

Follow-up Timing of Two Binary Pulsars with Massive White Dwarfs Discovered in Commensal Radio Astronomy FAST Survey

open access: yesThe Astrophysical Journal
We present phase-connected timing solutions, total-intensity and polarized profiles for two newly discovered pulsars, PSRs J1929+4105 and J2359+4239, identified by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio ...
D. Zhao   +39 more
doaj   +1 more source

Eclipsing Binary Pulsars

open access: yes, 2004
The first eclipsing binary pulsar, PSR B1957+20, was discovered in 1987. Since then, 13 other eclipsing low-mass binary pulsars have been found, 12 of these are in globular clusters. In this paper we list the known eclipsing binary pulsars and their properties, with special attention to the eclipsing systems in 47 Tuc.
openaire   +2 more sources

Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey

open access: yesThe Astrophysical Journal
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

An Alternative Explanation for the Helium Star Pulsar Binary J1928+1815: The Most Heavyweight Black Widow System to Date

open access: yesThe Astrophysical Journal
We present the results of deep near-infrared imaging of the recently discovered helium star pulsar binary J1928+1815 situated in the Galactic plane. Our observations did not achieve significant detections, providing limiting magnitudes of J = 23.7 and H =
Hang Gong   +9 more
doaj   +1 more source

The Anomalous Acceleration of PSR J2043+1711: Long-period Orbital Companion or Stellar Flyby?

open access: yesThe Astrophysical Journal
Based on the rate of change of its orbital period, PSR J2043+1711 has a substantial peculiar acceleration of 3.5 ± 0.8 mm s ^–1 yr ^–1 , which deviates from the acceleration predicted by equilibrium Milky Way (MW) models at a 4 σ level.
Thomas Donlon II   +55 more
doaj   +1 more source

Exploring Unusual High-frequency Eclipses in MSP J1908+2105

open access: yesThe Astrophysical Journal
This paper presents a comprehensive study of the eclipse properties of the spider millisecond pulsar (MSP) J1908+2105, using wide-band observations from the uGMRT and Parkes UWL. For the first time, we observed that this pulsar exhibits extended eclipses
Ankita Ghosh   +5 more
doaj   +1 more source

First Systematic Study Reporting the Changes in Eclipse Cutoff Frequency for Pulsar J1544+4937

open access: yesThe Astrophysical Journal
We present results from long-term monitoring of frequency-dependent eclipses of the radio emission from PSR J1544+4937, which is a black widow spider millisecond pulsar (MSP) in a compact binary system.
Sangita Kumari   +5 more
doaj   +1 more source

Orbital Trends of Binary Pulsars [PDF]

open access: yesSymposium - International Astronomical Union, 2004
We try to understand the eccentricity of high-mass binary pulsars using some methods of statistical mechanics.
openaire   +1 more source

Verification of f(R)-gravity in binary pulsars

open access: yesEPJ Web of Conferences, 2016
We develop the parameterized post-Keplerian approach for class of analytic f (R)-gravity models. Using the double binary pulsar system PSR J0737-3039 data we obtain restrictions on the parameters of this class of f (R)-models and show that f (R)-gravity ...
Dyadina Polina   +3 more
doaj   +1 more source

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