Results 201 to 210 of about 862,547 (224)
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2016
This work intends to contribute to the understanding of the radio emission of pulsars. Pulsars are neutron stars with a radius of about 10^6 cm and a mass of about one to three solar masses, that rotate with a period between seconds and milliseconds. They exhibit tremendous magnetic fields of 10^8 to 10^13 Gauss.
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This work intends to contribute to the understanding of the radio emission of pulsars. Pulsars are neutron stars with a radius of about 10^6 cm and a mass of about one to three solar masses, that rotate with a period between seconds and milliseconds. They exhibit tremendous magnetic fields of 10^8 to 10^13 Gauss.
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Journal of Physics G: Nuclear and Particle Physics, 2006
High-precision timing of radio pulsars in binary systems provides details of the current orbital parameters and usually suggests likely evolutionary histories. In the cases where general-relativistic corrections to the basic Keplerian orbit can be measured, the pulsar and companion masses can be inferred.
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High-precision timing of radio pulsars in binary systems provides details of the current orbital parameters and usually suggests likely evolutionary histories. In the cases where general-relativistic corrections to the basic Keplerian orbit can be measured, the pulsar and companion masses can be inferred.
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2006
Pulsars, rapidly rotating highly magnetized neutron stars, have many exciting applications in physics and astronomy. After nearly 40 years since the original discovery, pulsar research has great vitality, making major contributions to fields ranging from ultra-dense matter physics to relativistic gravity, cosmology and stellar evolution.
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Pulsars, rapidly rotating highly magnetized neutron stars, have many exciting applications in physics and astronomy. After nearly 40 years since the original discovery, pulsar research has great vitality, making major contributions to fields ranging from ultra-dense matter physics to relativistic gravity, cosmology and stellar evolution.
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2006
Radio pulsars are a major probe of the Galactic neutron star population and its evolution. Our attempts to derive the properties of the underlying, as opposed to the observed, population of radio pulsars in our Galaxy have gradually improved over the years thanks to large-scale surveys and more detailed simulations of the population.
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Radio pulsars are a major probe of the Galactic neutron star population and its evolution. Our attempts to derive the properties of the underlying, as opposed to the observed, population of radio pulsars in our Galaxy have gradually improved over the years thanks to large-scale surveys and more detailed simulations of the population.
openaire +1 more source
Binary and Millisecond Pulsars
Living Reviews in Relativity, 2008Duncan Lorimer, Lorimer Duncan R
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Spectral properties of 441 radio pulsars
Monthly Notices of the Royal Astronomical Society, 2018Ewan Barr, Matthew Kerr, Evan Keane
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Polarimetry of 600 pulsars from observations at 1.4 GHz with the Parkes radio telescope
Monthly Notices of the Royal Astronomical Society, 2018Matthew Kerr +2 more
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