PULSARS

作品数：382被引量：269H指数：7
导出分析报告
相关领域：天文地球更多>>
相关作者：王洪光杨信男更多>>
相关机构：中国科学院新疆天文台国家天文台北京大学广州大学更多>>
相关期刊：《Science China Mathematics》《Chinese Physics B》《Bulletin of the Chinese Academy of Sciences》《现代物理知识》更多>>
相关基金：国家自然科学基金国家重点基础研究发展计划国家高技术研究发展计划上海市自然科学基金更多>>
-
在结果中检索

检索结果分析

结果分析中...
选择条件：
  • 基金=国家重点基础研究发展计划（973Program）x
共 条 记 录，以下是1-5
全选清除导出
参考文献引证文献引用追踪
视图：
排序：
Simulation of the orbit and spin period evolution of the double pulsars PSR J0737-3039 from their birth to coalescence induced by gravitational wave radiation
《Research in Astronomy and Astrophysics》2021年第4期319-324,共6页Peng Liu Yi-Yan Yang Jian-Wei Zhang Maria Rah 
supported by the National Natural Science Foundation of China(NSFC,Grant Nos.11988101,11773005,U1631236,11703001,U1731238,U1938117,11725313,11721303);the International Partnership Program of Chinese Academy of Sciences(Grant No.114A11KYSB20160008);the National Key R&D Program of China(No.2016YFA0400702);supported by the National Basic Research Program(973 Program)(No.2015CB857100);National Key R&D Program of China(No.2017YFA0402600);the Guizhou Provincial Science and Technology Foundation(Grant No.[2020]1Y019)。
The complete orbital and spin period evolutions of the double neutron star(NS)system PSR J0737-3039 are simulated from birth to coalescence,which include the two observed radio pulsars classified as primary NS PSR J07...
关键词：PSR J0737–3039 double neutron star pulsar gravitational wave SIMULATION 
Reduced spin-down rate of PSR J0738–4042 explained as due to an asteroid disruption event
《Research in Astronomy and Astrophysics》2016年第5期41-46,共6页Yong-Bo Yu Yong-Feng Huang 
supported by the National Basic Research Program of China(973 Program,Grant No.2014CB845800);by the National Natural Science Foundation of China(Grant No.11473012)
Long term observations by Brook et al. reveal that the derivative of rotational frequency of PSR J0738-4042 changed abruptly in 2005. Originally, the spin-down rate was relatively stable, with the rotational frequency...
关键词：stars： neutron -- planet-star interactions -- pulsars： individual （PSR J0738-4042） 
Estimate of an environmental magnetic field of fast radio bursts
《Research in Astronomy and Astrophysics》2016年第3期11-16,共6页Wei-Li Lin Zi-Gao Dai 
supported by the National Basic Research Program ("973" Program) of China (Grant No. 2014CB845800);the National Natural Science Foundation of China (Grant No. 11033002)
Fast radio bursts （FRBs） are a type of newly-discovered transient astronomical phenomenon. They have short durations, high dispersion measures and a high event rate. However, due to unknown dis- tances and undetecte...
关键词：radio continuum： general -- pulsars： general -- galaxies： magnetic fields -- Galaxy： structure 
A note on the puzzling spindown behavior of the Galactic center magnetar SGR J1745-2900
《Research in Astronomy and Astrophysics》2015年第9期1467-1474,共8页Hao Tong 
supported by the Xinjiang Bairen project;the National Natural Science Foundation of China (NSFC, 11103021);West Light Foundation of CAS (LHXZ201201);Youth Innovation Promotion Association of CAS;the National Basic Research Program of China (973 Program, 2015CB857100)
SGR J1745-2900 is a magnetar near the Galactic center. X-ray observations of this source found a decreasing X-ray luminosity accompanied by an enhanced spindown rate. This negative correlation between X-ray luminosity...
关键词：pulsars： individual （SGR J1745-2900） -- stars： magnetar -- stars： neu-tron -- stars： winds 
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 
全选清除导出
共1页<1>
检索报告 对象比较 聚类工具 使用帮助 返回顶部