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Die Häufigkeit der Doppelsterne in der Sonnenumgebung

 

作者: P. Brosche,  

 

期刊: Astronomische Nachrichten  (WILEY Available online 1965)
卷期: Volume 288, issue 1‐3  

页码: 33-37

 

ISSN:0004-6337

 

年代: 1965

 

DOI:10.1002/asna.19652880108

 

出版商: WILEY‐VCH Verlag

 

数据来源: WILEY

 

摘要:

The observed relative frequency of visual double stars in the solar neighbourhood decreases with increasing distance. This diminution is quantitatively explained as result of the most efficient selection effect, which is caused by the resolving power of the great refractors. The observed values are in good agreement with such theoretical curves for which the true double star frequency is accepted to be 40% to 80%.

 

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