J
J. M. Yao
Researcher at Chinese Academy of Sciences
Publications - 4
Citations - 977
J. M. Yao is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Pulsar & Thick disk. The author has an hindex of 2, co-authored 4 publications receiving 651 citations.
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Journal ArticleDOI
A New Electron-density Model for Estimation of Pulsar and FRB Distances
TL;DR: In this article, a new model for the distribution of free electrons in the Galaxy, the Magellanic Clouds, and the intergalactic medium (IGM) that can be used to estimate distances to real or simulated pulsars and fast radio bursts (FRBs) based on their dispersion measure (DM) was presented.
Journal ArticleDOI
A New Electron Density Model for Estimation of Pulsar and FRB Distances
TL;DR: In this paper, a new model for the distribution of free electrons in the Galaxy, the Magellanic Clouds and the intergalactic medium (IGM) that can be used to estimate distances to real or simulated pulsars and fast radio bursts (FRBs) based on their dispersion measure (DM) is presented.
Journal ArticleDOI
Periodic and Phase-locked Modulation in PSR B1929+10 Observed with FAST
Fei-Fei Kou,W. M. Yan,Bo Peng,Ju-Fu Lu,Kai Liu,Kai Liu,Chun-sheng Zhang,Richard G. Strom,Richard G. Strom,Long Wang,Long Wang,Jian-Ping Yuan,Jian-Ping Yuan,R. Yuen,Y. Z. Yu,J. M. Yao,B. S. Liu,Jingzhi Yan,Peng Jiang,C. J. Jin,Di Li,Di Li,Lei Qian,Youling Yue,Yu-Xuan Zhu +24 more
Journal ArticleDOI
Periodic and Phase-locked Modulation in PSR B1929+10 Observed with FAST
Fei-Fei Kou,W. M. Yan,Bo Peng,Ju-Fu Lu,Kai Liu,Chun-sheng Zhang,Richard G. Strom,Long Wang,Jian-Ping Yuan,R. Yuen,Y. Z. Yu,J. M. Yao,B. S. Liu,Jingzhi Yan,Peng Jiang,C. J. Jin,Di Li,Lei Qian,Youling Yue,Yu-Xuan Zhu +19 more
TL;DR: In this paper, a detailed single-pulse analysis for PSR B1929+10 is presented based on observations with the Five-hundred-meter Aperture Spherical radio Telescope (FAST), where the main pulse and interpulse are found to be modulated with a periodicity of 12 times the pulsar's rotational period.