Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Guo Jun Qiao"'
Autor:
Jun-Tao, Bai, Xin, Xu, Quan-Wei, Lin, Qi-Jun, Zhi, Lun-Hua, Shang, Yuan-Jie, Du, You-Li, Tuo, Shi-Jun, Dang, Shuang-Qiang, Wang, Ru-Shuang, Zhao, Ai-Jun, Dong, Guo-Jun, Qiao
Publikováno v:
In New Astronomy February 2021 83
Autor:
Ji-feng Liu, Guo-jun Qiao
Publikováno v:
Chinese Astronomy and Astrophysics. 23:133-138
Empirical theory of pulsar radio emission emphasized that the emission beam consists of a central core and two concentric cones and pointed out that there exists two distinct trends in mean pulse profile evolution: the profile width increases in one
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::400f1eef91b7cf2e331e9926dcd92da7
https://doi.org/10.1016/s0275-1062(99)00036-3
https://doi.org/10.1016/s0275-1062(99)00036-3
Publikováno v:
Chinese Astronomy and Astrophysics. 19:432-439
The successes and shortcomings of the magnetic dipole emission model of pulsars are reviewed and a modification of the model presented. A power-law relation is found statistically between the modifying factor and the time derivative of the period. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a14ae7c6604e4aa4473a8366fa1a390b
https://doi.org/10.1016/0275-1062(95)00059-2
https://doi.org/10.1016/0275-1062(95)00059-2
Autor:
Guo Jun Qiao, Yuan Jie Du
The multi-wavelength pulsed emission from young pulsars and millisecond pulsars can be well modeled with the single-pole 3-dimension annular gap and core gap model. To distinguish our single magnetic pole model from two-pole models (e.g. outer gap mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e29706e87e382a8c8caad9a80635e2c
http://arxiv.org/abs/1210.5801
http://arxiv.org/abs/1210.5801
Autor:
Lun-Hua Shang, Ji-Guang Lu, Yuan-Jie Du, Long-Fei Hao, Di Li, Ke-Jia Lee, Bin Li, Li-Xin Li, Guo-Jun Qiao, Zhi-Qiang Shen, De-Hua Wang, Min Wang, Xin-Ji Wu, Ya-Jun Wu, Ren-Xin Xu, You-Ling Yue, Zhen Yan, Qi-Jun Zhi, Rong-Bing Zhao, Ru-Shuang Zhao
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jul2017, Vol. 468 Issue 4, p4389-4398, 10p
Akademický článek
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Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
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Autor:
Ru-Shuang Zhao, Zhen Yan, Xin-Ji Wu, Zhi-Qiang Shen, R. N. Manchester, Jie Liu, Guo-Jun Qiao, Ren-Xin Xu, Ke-Jia Lee
Publikováno v:
Astrophysical Journal; 3/20/2019, Vol. 874 Issue 1, p1-1, 1p
Autor:
Hong-Guang Wang, Guo-Jun Qiao, Yuan-Jie Du, Ji-Guang Lu, Ren-Xin Xu, Ke-Jia Lee, Xiong-Wei Liu
Publikováno v:
Research in Astronomy & Astrophysics; Feb2019, Vol. 19 Issue 2, p1-1, 1p
Autor:
Guo-Jun Qiao, Jiu-Heng Cheng
Publikováno v:
The Astrophysical Journal. 340:503
Hercules X-1 exhibits a 35 day cycle in its X-ray intensity and 1.24 s and 1.7 day periodicities in its pulsar rotation and orbit, respectively. The features of the 35 day clock and the presence of a precessing tilted accretion disk have been discuss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8f516bc78ab99fff73831a718ee10f11
https://doi.org/10.1086/167412
https://doi.org/10.1086/167412