Neutron Star Kicks in Isolated and Binary Pulsars: Observational Constraints and Implications for Kick Mechanisms [PDF]
Chen Wang, Dong Lai, J. L. Han
openalex +1 more source
An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers. [PDF]
Pang PTH +20 more
europepmc +1 more source
We have searched for radio pulsations toward 49 Fermi Large Area Telescope (LAT) 1FGL Catalog γ -ray sources using the Green Bank Telescope at 350 MHz. We detected 18 millisecond pulsars (MSPs) in blind searches of the data; 10 of these were discoveries ...
P. Bangale +20 more
doaj +1 more source
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Annala E +6 more
europepmc +1 more source
HYDRODYNAMICS OF INTERACTION OF PULSAR AND STELLAR WINDS AND ITS IMPACT ON THE HIGH ENERGY RADIATION OF BINARY PULSAR SYSTEMS [PDF]
D. Khangulyan +4 more
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An Approach for Estimating the Deformation of Pulsar Included in Binary-System PSR B 1913+16 [PDF]
Mohammed Mohammed Soleiman +3 more
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Can Slow Pulsars in Milky Way Globular Clusters Form via Partial Recycling?
Alongside the population of several hundred radio millisecond pulsars currently known in Milky Way globular clusters, a subset of six slowly spinning pulsars (spin periods 0.3–4 s) are also observed.
Kyle Kremer +5 more
doaj +1 more source
The Green Bank Northern Celestial Cap Pulsar Survey. VI. Timing and Discovery of PSR J1759+5036: A Double Neutron Star Binary Pulsar [PDF]
Gabriella Agazie +29 more
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Recovering Pulsar Periodicity from Time-of-arrival Data by Finding the Shortest Vector in a Lattice
The strict periodicity of pulsars is one of the primary ways through which their nature and environment can be studied, and it has also enabled precision tests of general relativity and studies of nanohertz gravitational waves using pulsar timing arrays (
Dotan Gazith +2 more
doaj +1 more source
Identifying Companions in Pulsar Binary Systems via Gaia Data
In the optical band, very few pulsars can be directly detected, but some of the pulsar binary companions can be observed. This study leverages high-precision astrometric data from Gaia Data Release 3 (DR3) to identify pulsar companions in binary systems.
Yueqi Song +5 more
doaj +1 more source

