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A NUMERICAL ANALYSIS OF THE VARIATION OF THE ORBITAL PERIOD AND THE PHYSICAL MECHANISM OF FLUCTUATION OF THE LIGHT CURVE OF THE CLOSE BINARY VW CEP
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作者 刘学富 罗承忠 +1 位作者 芦圣治 孙岳 《Chinese Science Bulletin》 SCIE EI CAS 1981年第12期1096-1101,共6页
Ⅰ. INTRODUCTION The close binary VW Cep is a contact pair of the W-type UMa. Its period is 0.2783 days; spectrum G5+K1; and mass 1.1m_☉+0.4m_☉. Since astronomer Schilt discovered it in 1927, for the past fifty year... Ⅰ. INTRODUCTION The close binary VW Cep is a contact pair of the W-type UMa. Its period is 0.2783 days; spectrum G5+K1; and mass 1.1m_☉+0.4m_☉. Since astronomer Schilt discovered it in 1927, for the past fifty years and more, its luminosity, spectrum and 展开更多
关键词 LUMINOSITY fifty BRIGHTNESS orbital stars rotation instr NEIGHBORHOOD LISTED SPOTS
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