Results 151 to 160 of about 809,546 (293)
Spectral Studies of Super‐Eddington Accreting Neutron Stars in the Magellanic Clouds
ABSTRACT Major outbursts of BeXRBs offer a unique laboratory for studying accretion onto magnetized neutron stars (NSs) over a large dynamic range. The accreting material is entrained from the accretion disk by the strong magnetic field, and then channeled onto the NS, forming a so‐called accretion column (AC).
Georgios Vasilopoulos +3 more
wiley +1 more source
Binary Pulsars: Observations and Implications [PDF]
The Galaxy contains a large number of neutron stars in gravitation-ally bound binary systems. Among the most fruitful of these to study have been the binary radio pulsars, of which seven are now known. Unlike the “accretion-powered” neutron stars located in mass-exchanging X-ray binary systems, the “rotation-powered” binary radio pulsars are found in ...
openaire +1 more source
Binary and Millisecond Pulsars
We review the main properties, demographics and applications of binary and millisecond radio pulsars. Our knowledge of these exciting objects has greatly increased in recent years, mainly due to successful surveys which have brought the known pulsar ...
Lorimer Duncan R.
doaj
Radio Observations of a Candidate Redback Millisecond Pulsar: 1FGL J0523.5-2529
Redback pulsars are a subclass of millisecond pulsar system with a low-mass non-degenerate companion star being ablated by the pulsar. They are of interest due to the insights they can provide for late-stage pulsar evolution during the recycling process.
Owen. A. Johnson +6 more
doaj +1 more source
Gravitational wave astronomy of single sources with a pulsar timing array
Abbreviated: We investigate the potential of detecting the gravitational wave from individual binary black hole systems using pulsar timing arrays (PTAs) and calculate the accuracy for determining the GW properties.
B. W. Stappers +61 more
core +1 more source
A Lower Mass Estimate for PSR J0348+0432 Based on CHIME/Pulsar Precision Timing
The binary pulsar J0348+0432 was previously shown to have a mass of approximately 2 M _⊙ , based on the combination of radial-velocity and model-dependent mass parameters derived from high-resolution optical spectroscopy of its white-dwarf companion.
Alexander Saffer +10 more
doaj +1 more source
Investigation for Binary Characteristics of LS I + 61°303 with Optical Polarization
We investigate the optical linear polarization caused by Thomson scattering of the stellar radiation for gamma-ray binary LS I + 61°303, which likely contains a young pulsar.
Jiaxin Liu +5 more
doaj +1 more source
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
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
Testing Gravity with Binary Pulsars in the SKA Era
Binary (and trinary) radio pulsars are natural laboratories in space for understanding gravity in the strong field regime, with many unique and precise tests carried out so far, including the most precise tests of the strong equivalence principle and of ...
Vivek Venkatraman Krishnan +23 more
doaj +1 more source

