Median Statistics Estimate of the Distance to the Galactic Center

被引:45
|
作者
Camarillo, Tia [1 ]
Mathur, Varun [1 ,2 ]
Mitchell, Tyler [1 ]
Ratra, Bharat [1 ]
机构
[1] Kansas State Univ, Dept Phys, 116 Cardwell Hall, Manhattan, KS 66506 USA
[2] Birla Inst Technol & Sci, Dept Phys, Pilani 403726, Goa, India
基金
美国国家科学基金会;
关键词
distance scale; Galaxy: fundamental parameters; methods: data analysis; methods: statistical; SOLAR GALACTOCENTRIC DISTANCE; ROTATION; CONSTRAINTS; KINEMATICS; VARIABLES; AGE;
D O I
10.1088/1538-3873/aa9b26
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that error distributions of a compilation of 28 recent independent measurements of the distance from the Sun to the Galactic center, R-0, are wider than a standard Gaussian and best fit by an n=4 Student's t probability density function. Given this non-Gaussianity, the results of our median statistics analysis, summarized as R-0 = 8.0 +/- 0.3 kpc (2 sigma error), probably provides the most reliable estimate of R-0.
引用
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页数:10
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