Journal of Astronomy and Space Sciences

The Korean Space Science Society (한국우주과학회)
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THE MASS AND ANGULAR MOMENTUM RELATION OF ECLIPSING BINARIES

식쌍성의 질량과 궤도 각운동량 관계

  • Oh, Kyu-Dong (Department of Earth Science Education, Chonnam National University)
  • 오규동 (전남대학교 지구과학교육과)
  • Published : 1998.06.01
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Abstract

With a total 2780 eclipsing binary systems in the Catalogue of Approximate Photometric and Absolute Elements of Eclipsing Variable Stars by Svechnikov & Kuznetsova(1990), the empirical relations between the systemic mass and orbital argular momentum have been examined. It is found that, during the its evolution, the total orbital argular momentum of the eclipsing binary sustem is not conserved. It decreases gradually, though not at a constant rate, until the system becomes into contact from initially detached via semi-detached system.

Svechnikow & Kuznetsova (1990)의 Catalogue of Approximate Photometric and Absolute Elements of Eclipsing Variable로 부토 3780개의 식 쌍성들을 이용하여 식 쌍성의 질량-궤도 각 운동량과의 상관 관계를 조사하였다. 그 결과 쌍성이 진화하는 동안 궤도 각 운동량이 보전되지 못하며, 비록 일정한 값을 갖지는 않지만 점진적으로 분리형에서 준분리 형으로 그리고 접촉형으로 진화할수록 그 값이 감소하는 것으로 나타났다.

Keywords

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