国家自然科学基金(s10935001)

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相关主题：PULSARSNEUTRON_STARSMAGNETARSGENERALEXCESS更多>>
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The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model
《Research in Astronomy and Astrophysics》2011年第12期1371-1376,共6页Hao Tong Ren-Xin Xu Li-Ming Song 
supported by the National Natural Science Foundation of China (NSFC, GrantNos. 10935001 and 10973002);the National Basic Research Program of China (973 Program, Grant No. 2009CB824800);the John Templeton Foundation
X-ray dim isolated neutron stars are peculiar pulsar-like objects, characterized by their Planck-like spectrum. In studying their spectral energy distributions, optical/ultraviolet （UV） excess is a long standing pro...
关键词：pulsars： individual （RX J0420.0-5022 RX J0720.4-3125 RX J0806.4-4123 RX J1308.6＋2127 RX J1605.3＋3249 RX J1856.5-3754 RX J2143.0＋0654）-- stars： neutron 
Pulsating magneto-dipole radiation of a quaking neutron star powered by energy of Alfvn seismic vibrations
《Research in Astronomy and Astrophysics》2011年第9期1085-1092,共8页Sergey Bastrukov Jun-Wei Yu Ren-Xin Xu Irina Molodtsova 
supportde by the National Natural Science Foundation of China(Grant Nos.10935001 and 10973002);the National Basic Research Program of China(Grant No.2009CB824800);the John Templeton Foundation
We compute the characteristic parameters of the magneto-dipole radiation of a neutron star undergoing torsional seismic vibrations under the action of Lorentz restoring force about an axis of a dipolar magnetic field ...
关键词：neutron stars -- torsion Alfv6n vibrations -- vibration powered radiation -- magnetic field decay -- magnetars 
A note on the discovery of a 2M_⊙ pulsar
《Research in Astronomy and Astrophysics》2011年第6期687-691,共5页Xiao-Yu Lai Ren-Xin Xu 
supported by the National Natural Science Foundation of China (Grant Nos. 10935001 and 10973002);the National Basic Research Program of China (973 program, Grant No. 2009CB824800);the China Postdoctoral Science Foundation and the John Templeton Foundation
It is conventionally thought that the state equation of dense matter softens and thus cannot result in high maximum mass if pulsars are quark stars and that a recently discovered 2M⊙ pulsar （PSR J1614–2230） may ma...
关键词：dense matter — elementary particles — pulsars： general — stars： neutron 
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