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Star-Disk Interactions in Multiband Photometric Monitoring of the Classical T Tauri Star GI Tau 期刊论文
ASTROPHYSICAL JOURNAL, 2018, 卷号: 852, 期号: 1, 页码: 56
Authors:  Guo, Zhen;  Herczeg, Gregory J.;  Jose, Jessy;  Fu, Jianning;  Chiang, Po-Shih;  Grankin, Konstantin;  Michel, Raul;  Yadav, Ram Kesh;  Liu, Jinzhong;  Chen, Wen-ping;  Li, Gang;  Xue, Huifang;  Niu, Hubiao;  Subramaniam, Annapurni;  Sharma, Saurabh;  Prasert, Nikom;  Flores-Fajardo, Nahiely;  Castro, Angel;  Altamirano, Liliana
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Stars: Pre-main Sequence  Stars: Variables: t Tauri  Herbig Ae/be  
The effects of the Reimers eta on the solar rotational period when our Sun evolves to the RGB tip 期刊论文
ASTROPHYSICS AND SPACE SCIENCE, 2017, 卷号: 362, 期号: 1, 页码: 15
Authors:  Guo, Jianpo;  Lin, Ling;  Bai, Chunyan;  Liu, Jinzhong
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Sun: Rotation  Stars: Mass Loss  Ism: Planetary Nebulae  Planets: Hot Jupiter  
Short timescale intensity fluctuations of PSR B1133+16 and PSR B1237+25 due to interstellar scintillation at 1.54 GHz 期刊论文
ASTROPHYSICS AND SPACE SCIENCE, 2013, 卷号: 347, 期号: 2, 页码: 327-335
Authors:  Niu, H. B.;  Esamdin, A.;  Wang, N.
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Ism: Pulsars: Individual: Psr b1237+25 Psr b1133+16  
Two-component scattering model and the electron density spectrum 期刊论文
ASTROPHYSICS AND SPACE SCIENCE, 2010, 卷号: 325, 期号: 2, 页码: 241-249
Authors:  Zhou, A. Z.;  Tan, J. Y.;  Esamdin, A.;  Wu, X. J.
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Stars: Pulsars: General  Radio Continuum: Stars  Ism: Structure  Scattering  
Two-component model for the interstellar scattering in direction to the Vela pulsar 期刊论文
ASTRONOMY & ASTROPHYSICS, 2005, 卷号: 438, 期号: 3, 页码: 909-914
Authors:  Zhou, AZ;  Esamdin, A;  Wu, XJ
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Stars : Pulsars : Individual : Psr B0833-45  Radio Continuum : Stars  Ism : Structure  Scattering  
A study of the long-term flux density variation of PSRs B0329+54 and B1508+55 期刊论文
ASTRONOMY & ASTROPHYSICS, 2004, 卷号: 425, 期号: 3, 页码: 949-954
Authors:  Esamdin, A;  Zhou, AZ;  Wu, XJ
Adobe PDF(172Kb)  |  Favorite  |  View/Download:170/0  |  Submit date:2015/08/25
Stars : Pulsars : Individual :  Ism : Structure  Psr b0329+54  Plasmas  Psr b1508+55  Turbulence