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Journal of Astronomy and Space Sciences
Article . 2003 . Peer-reviewed
Data sources: Crossref
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Journal of Astronomy and Space Sciences
Article
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SMALL MASS RATIO CONTACT BINARY

질량비가 작은 접촉쌍성
Authors: Kyu-Dong Oh; Chun-Hwey Kim; Young Woon Kang; Yonggi Kim;

SMALL MASS RATIO CONTACT BINARY

Abstract

The contact binary system has been classified in five different types according to their physical properties. We suggest that extremely small mass ratio contact binary systems(q<0.2) could be classified as a new type of contact binaries in addition to the classification. According to the Svechnikov & Kuznetsova (1990)'s catalogue, the spectral types of primary components of newly classified contact binaries are distributed at A type, and also the distribution of their various physical characteristics is laid at the center region dividing the early-type contact binaries from late-type contact binaries.

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Keywords

classification, Astronomy, contact binary, QB1-991, small mass ratio contact bianry

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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