Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Du, Yuanjie"'
Publikováno v:
In Case Studies in Thermal Engineering January 2025 65
Akademický článek
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Autor:
Du, Yuanjie, Qiao, Guojun, Shuai, Ping, Bei, Xiaomin, Chen, Shaolong, Fu, Linzhong, Huang, Liangwei, Lin, Qingqing, Meng, Jing, Wu, Yaojun, Zhang, Hengbin, Zhang, Qian, Zhang, Xinyuan
Publikováno v:
ApJ, 801, 131 (2015)
PSR B1821$-$24 is a solitary millisecond pulsar (MSP) which radiates multi-wavelength pulsed photons. It has complex radio, X-ray and $\gamma$-ray pulse profiles with distinct peak phase-separations that challenge the traditional caustic emission mod
Externí odkaz:
http://arxiv.org/abs/1501.02867
Publikováno v:
ApJ, 782, L38 (2014)
PSR J0218$+$4232 is a millisecond pulsar (MSP) with a flux density $\sim$ 0.9 mJy at 1.4 GHz. It is very bright in the high-energy X-ray and $\gamma$-ray domains. We conducted an astrometric program using the European VLBI Network (EVN) at 1.6 GHz to
Externí odkaz:
http://arxiv.org/abs/1402.2380
Publikováno v:
ApJ, 763, 29 (2013)
Pulsed gamma-ray emission from millisecond pulsars (MSPs) has been detected by the sensitive Fermi, which sheds light on studies of the emission region and mechanism. In particular, the specific patterns of radio and gamma-ray emission from PSR J0101
Externí odkaz:
http://arxiv.org/abs/1211.5208
Autor:
Qiao, Guojun, Liu, Xiongwei, Xu, Renxin, Du, Yuanjie, Han, Jinlin, Tong, Hao, Wang, Hongguang
The concept of a "magnetar" was proposed mainly because of two factors. First, the X-ray luminosity of Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Ray Repeaters (SGRs) is larger than the rotational energy loss rate, and second, the magnetic field s
Externí odkaz:
http://arxiv.org/abs/1211.3298
Autor:
Du, YuanJie, Qiao, GuoJun
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:
http://arxiv.org/abs/1210.5801
Publikováno v:
ApJ, 2012, 748, 84
In the framework of the three-dimensional (3D) annular gap model with reasonable parameters (the magnetic inclination angle \alpha = 45 deg and the view angle \zeta = 63 deg), we first use the latest hight energy data to self-consistently calculate r
Externí odkaz:
http://arxiv.org/abs/1202.1096
Pulsars have been recognized as normal neutron stars or quark stars. Sub-millisecond pulsars, if detected, would play an essential and important role in distinguishing quark stars from neutron stars. A key question is how sub-millisecond pulsars coul
Externí odkaz:
http://arxiv.org/abs/0803.1334
Akademický článek
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