Results 11 to 20 of about 809,546 (293)
A binary pulsar in a 53-minute orbit. [PDF]
Nature, 2023 PSR J1953+1844 (M71E) has an orbital period of 53.3 minutes and a companion with a mass of 0.07 M _⊙, making it a bridging object between redbacks and black widows in the evolutionary track. Spider pulsars are neutron stars that have a companion star in
Pan Z +17 more
europepmc +2 more sources
Modulated Gamma-ray emission from compact millisecond pulsar binary systems [PDF]
, 2013 A significant amount of the millisecond pulsars has been discovered within binary systems. In several such binary systems the masses of the companion stars have been derived allowing to distinguish two classes of objects, called the Black Widow and the ...
Bednarek, W.
core +2 more sources
A timing formula for main-sequence star binary pulsars [PDF]
, 1997 In binary radio pulsars with a main-sequence star companion, the spin-induced quadrupole moment of the companion gives rise to a precession of the binary orbit.
Wex, N.
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A Massive Pulsar in a Compact Relativistic Binary [PDF]
Science, 2013 Introduction Neutron stars with masses above 1.8 solar masses (M☉), possess extreme gravitational fields, which may give rise to phenomena outside general relativity.
John Antoniadis +2 more
exaly +2 more sources
Overcoming the Challenges of Transmural Durable Lesions With PFA-Impact of Electrode Design and Contact Assessment. [PDF]
Pacing Clin ElectrophysiolAbstract Electrode design and reliable contact assessment are critical for creating durable pulsed field ablation (PFA) lesions to treat atrial fibrillation while minimizing collateral damage. This review introduces a novel “map‐and‐ablate” PFA catheter featuring flat electrodes, thermal contact assessment, and fully customizable electrode selection ...
Melki L, Moisa S, Reinders D, Boucher S.
europepmc +2 more sources
Proton Acceleration with Relativistic Electromagnetic Shock. [PDF]
Adv Sci (Weinh)New Ion Acceleration Mechanism! A novel cosmic‐ray proton acceleration mechanism is proposed, where relativistic electromagnetic shocks accelerate protons transversely. Hamiltonian analysis yields a scaling law linking the proton energy to the minimum longitudinal thickness of the shock.
Xiao T +5 more
europepmc +2 more sources
1974: the discovery of the first binary pulsar [PDF]
, 2015 The 1974 discovery, by Russell A. Hulse and Joseph H. Taylor, of the first binary pulsar PSR B1913+16, opened up new possibilities for the study of relativistic gravity.
Damour, Thibault
core +3 more sources
A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437–4715 [PDF]
The Astrophysical Journal LettersWe report Bayesian inference of the mass, radius, and hot X-ray emitting region properties—using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest rotation-powered millisecond X-ray pulsar, PSR J0437−4715. Our modeling is
Devarshi Choudhury +19 more
doaj +2 more sources
SOME EVOLUTIONARY ASPECTS OF THE BINARY STELLAR SYSTEMS CONTAINING NEUTRON STAR
Odessa Astronomical Publications, 2012 The obvious lack of the binary stellar systems that contain neutron stars (NS) is observed at present. Partly it is caused by the fact that it is very difficult to detect neutron star in a binary system if this relativistic component does not manifest ...
Oleg O. Ulyanov +3 more
doaj +3 more sources
Binary and Millisecond Pulsars
Living Reviews in Relativity, 2008 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 +2 more sources