Statistical study of visual binaries
- 作者: Abdel-Rahman H.I.1,2, Nouh M.I.1,3, Elsanhoury W.H.1,3
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隶属关系:
- National Research Institute of Astronomy and Geophysics
- Shaqra University
- Northern Border University
- 期: 卷 72, 编号 2 (2017)
- 页面: 199-205
- 栏目: Article
- URL: https://journal-vniispk.ru/1990-3413/article/view/212444
- DOI: https://doi.org/10.1134/S1990341317020110
- ID: 212444
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详细
In this paper, some statistical distributions of wide pairs included in the Washington Double Star Catalog are investigated. Frequency distributions and testing hypothesis are derived for some basic parameters of visual binaries. It was found that the magnitude difference is distributed exponentially, which means that the majority of the components of the selected systems are of the same spectral type. The distribution of mass ratios is concentrated at about 0.7 which agrees with Salpeter mass function. The distribution of the linear separation appears to be exponential which contradicts previous studies for close binaries.
作者简介
H. Abdel-Rahman
National Research Institute of Astronomy and Geophysics; Shaqra University
编辑信件的主要联系方式.
Email: helal_ismaeil@yahoo.com
埃及, Cairo, 11421; Shaqra, 11961
M. Nouh
National Research Institute of Astronomy and Geophysics; Northern Border University
Email: helal_ismaeil@yahoo.com
埃及, Cairo, 11421; Arar, 73222
W. Elsanhoury
National Research Institute of Astronomy and Geophysics; Northern Border University
Email: helal_ismaeil@yahoo.com
埃及, Cairo, 11421; Arar, 73222
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