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The phenomenon of pulsar nulling, where pulsars temporarily and stochastically cease their radio emission, is thought to be indicative of a “dying” pulsar, where radio emission ceases entirely.
Garvit Grover+6 more
doaj +1 more source
Theoretical Implications of the 47 Tuc Pulsars [PDF]
Twenty millisecond radio pulsars have now been observed in the globular cluster 47 Tuc. This is by far the largest sample of radio pulsars known in any globular cluster. These recent observations provide a unique opportunity to re-examine theoretically the formation and evolution of recycled pulsars in globular clusters.
arxiv
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openaire +3 more sources
Polarization characteristics of southern pulsars - I. 400-MHz observations [PDF]
P. A. Hamilton+3 more
openalex +1 more source
Angular size of the Crab Pulsar at 74 MHz [PDF]
W. A. Coles, J. J. Kaufman
openalex +1 more source
On the overall properties of young neutron stars: an application to the Crab pulsar
In this brief report, we present a model that complements the well-established canonical model for the spin evolution of rotation-powered pulsars, which is typically used to estimate ages, spin-down luminosity, and surface magnetic fields of middle-aged ...
Cristian G. Bernal+8 more
doaj +1 more source
Polarization characteristics of southern pulsars - II. 640-MHz observations [PDF]
P. M. McCulloch+3 more
openalex +1 more source
Serendipitous Discovery of a 431 ms Pulsar in the Background of Westerlund 1
We report the discovery of PSR J1646−4545, a 431 ms isolated pulsar, in the direction of the young massive cluster Westerlund 1. The pulsar was found in data taken between the years 2005 and 2010 with the “Murriyang” Parkes radio telescope in Australia ...
Viviana Piga+8 more
doaj +1 more source