EFFECTIVE TEMPERATURE OF OV STARS

OV 별의 유효온도

  • Cho, Soon-Wha (Department of Science Education, Graduate School, Seoul National University) ;
  • Yun, Hong-Sik (Department of Astronomy, College of Natural Sciences, Seoul National University)
  • 조순화 (서울대학교 대학원 과학교육과 지학교육) ;
  • 윤홍식 (서울대학교 자연과학대학 천문학과)
  • Published : 1977.12.31

Abstract

$Str\ddot{o}mgren$-system colors for 23 OV stars compiled by Crawford have been compared with colors calculated by Mihalas from non-LTE model atmospheres. In this way, effective temperatures of these stars have been determined and plotted against spectral type, $c_1$ (u-b), (b-y), (U-B), and (B-V). Within the accuracy of the observations, effective temperatures derived from the photometry for these 23 main-sequence stars are found to be in good agreement with Contiis spectroscopical temperatures.

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