Results 171 to 180 of about 6,438 (185)

Progress and prospects in high energy astrophysics. [PDF]

Proc Natl Acad Sci U S A, 1975
Rees MJ.
europepmc   +1 more source

The Astrobiology Primer v2.0. [PDF]

Astrobiology, 2016
Domagal-Goldman SD, Wright KE, Adamala K, Arina de la Rubia L, Bond J, Dartnell LR, Goldman AD, Lynch K, Naud ME, Paulino-Lima IG, Singer K, Walther-Antonio M, Abrevaya XC, Anderson R, Arney G, Atri D, Azúa-Bustos A, Bowman JS, Brazelton WJ, Brennecka GA, Carns R, Chopra A, Colangelo-Lillis J, Crockett CJ, DeMarines J, Frank EA, Frantz C, de la Fuente E, Galante D, Glass J, Gleeson D, Glein CR, Goldblatt C, Horak R, Horodyskyj L, Kaçar B, Kereszturi A, Knowles E, Mayeur P, McGlynn S, Miguel Y, Montgomery M, Neish C, Noack L, Rugheimer S, Stüeken EE, Tamez-Hidalgo P, Imari Walker S, Wong T.   +48 more
europepmc   +1 more source

Varying Constants, Gravitation and Cosmology. [PDF]

Living Rev Relativ, 2011
Uzan JP.
europepmc   +1 more source

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Rotation and Accretion Powered Pulsars

Physics Today, 2008
Buchbesprechung (Rotation and accretion powered pulsars, Pranab Ghosh, World Scientific, Hackensack, NJ, 2007)
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Rotation and Accretion Powered Pulsars

Classical and Quantum Gravity, 2008
Pulsar astrophysics has come a long way in the 40 years since the discovery of the first pulsar by Bell and Hewish. From humble beginnings as bits of 'scruff' on the Cambridge University group's chart recorder paper, the field of pulsars has blossomed into a major area of mainstream astrophysics, with an unparalleled diversity of astrophysical ...
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High-Energy Emission From Rotation-Powered Pulsars

AIP Conference Proceedings, 2008
Forty years after the discovery of rotation‐powered pulsars, we still do not understand many aspects of their pulsed emission. In the last few years there have been some fundamental developments in acceleration and emission models. I will review both the basic physics of the models as well as the latest developments in understanding the high‐energy ...
Alice K. Harding, Ye-Fei Yuan, Xiang-Dong Li, Dong Lai   +3 more
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X-Ray Emission from Rotation-Powered Pulsars

Chinese Physics Letters, 2005
We study the properties of pulsed component of hard (2–10 keV) x-ray emission from pulsars based on the new version of outer gap model we proposed previously [Astrophys. J. 604 (2004) 317]. On the frame of this outer gap model, we derive an expression of non-thermal pulsed x-ray luminosity of rotation-powered pulsars, and then apply it to the pulsars ...
Lin Gui-Fang, Zhang Li
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Rotation and Accretion Powered Pulsars

2007
The Discovery of Pulsars Physics of Neutron Stars Origin and Evolution of Neutron Stars Properties of Rotation Powered Pulsars Superfluidity in Neutron Stars and Glitch Diagnostics Properties of Accretion Powered Pulsars Pulsar Magnetospheres Pulsar Emission Mechanisms Spin Evolution of Neutron Stars Neutron Star Magnetic Fields Strange Stars.
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Luminosity Evolution of Rotation-Powered, High-Energy Pulsars

Proceedings of the 12th Asia Pacific Physics Conference (APPC12), 2014
We investigate the pulsar outer-magnetospheric particle accelerator and derive how the trans-magnetic-field thickness of the accelerator evolves with the pulsar age. We find that the thickness is small but increases steadily if the neutron-star envelope is contaminated by sufficient light elements.
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Rotation Powered Pulsars as Sources of High-Energy Particles

2007
Highly magnetised rapidly spinning neutron stars are widely considered to be natural sites for acceleration of charged particles. A powerful acceleration mechanism due to unipolar induction is thought to operate in the magnetospheres of isolated neutron stars, bringing the particles to ultrarelativistic energies at the expense of the neutron star ...
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