Results 131 to 140 of about 3,124 (236)

Recovering Pulsar Braking Index from a Population of Millisecond Pulsars

open access: yesThe Astrophysical Journal
The braking index, n , of a pulsar is a measure of its angular momentum loss and the value it takes to correspond to different spin-down mechanisms. For a pulsar spinning down due to gravitational-wave emission from the principal mass quadrupole mode ...
A. L. Hewitt, M. Pitkin, I. M. Hook
doaj   +1 more source

CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]

open access: yesAstrophys J, 2017
Wadiasingh Z   +4 more
europepmc   +1 more source

Formation of binary millisecond pulsars by accretion-induced collapse of white dwarfs [PDF]

open access: bronze, 2009
Jarrod R. Hurley   +4 more
openalex   +1 more source

Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]

open access: yesNat Astron, 2022
Caleb M   +21 more
europepmc   +1 more source

Optical polarization curve of the transitional millisecond pulsar PSR J1023+0038 during an X-ray flaring mode. [PDF]

open access: green
M. C. Baglio   +19 more
openalex   +1 more source

Radio Observations of a Candidate Redback Millisecond Pulsar: 1FGL J0523.5-2529

open access: yesThe Open Journal of Astrophysics
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

Radio Pulse Properties of the Millisecond Pulsar PSR J0437-4715

open access: green, 1998
F. A. Jenet   +4 more
openalex   +2 more sources

The Parkes Multibeam Pulsar Survey - V. Finding binary and millisecond pulsars [PDF]

open access: bronze, 2004
A. J. Faulkner   +11 more
openalex   +1 more source

Eccentric Binary Millisecond Pulsars

open access: yes, 2009
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

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