| A Kinematical Calibration of the Galactocentric Distance |
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| 引用本文： | Ming Shen and Zi Zhu Department of Astronomy,Nanjing University,Nanjing 210093,. A Kinematical Calibration of the Galactocentric Distance[J]. 中国天文和天体物理学报, 2007, 7(1): 120-128 |
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| 作者姓名： | Ming Shen and Zi Zhu Department of Astronomy Nanjing University Nanjing 210093 |
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| 作者单位： | Ming Shen and Zi Zhu Department of Astronomy，Nanjing University，Nanjing 210093; |
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| 摘 要： | 1 INTRODUCTION The distance to the Galactic center R0 is a fundamental constant for astronomy and astrophysics. Most determinations of astronomical quantities are directly connected with the Galactic distance scale, e.g., the rotational speed of our Galax…
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| 关 键 词： | Galaxy: kinematics and dynamics—stars: early-type—open clusters and associations |
A Kinematical Calibration of the Galactocentric Distance |
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| Ming Shen,Zi Zhu. A Kinematical Calibration of the Galactocentric Distance[J]. Chinese Journal of Astronomy and Astrophysics, 2007, 7(1): 120-128 |
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| Authors: | Ming Shen Zi Zhu |
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| Affiliation: | Department of Astronomy, Nanjing University, Nanjing 210093 |
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| Abstract: | |
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| Keywords: | Galaxy: kinematics and dynamics - stars: early-type - open clusters and associations |
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