NAOC Open IR
WYCnC的四色uvby测光和食外畸变波的黑子模拟
李炎; 解兴发; 翟迪生; 陈海林
1989
Source Publication天体物理学报
ISSN0253-2379
Volume9Issue:2Pages:97
Abstract作者于1986年3月间,对短周期RS CVn型双星WY Cnc进行了uvby四色光电观测。采用改进了的包含黑子微分改正的W-D程序,对b和y光变曲线,以及Chambliss 1965年发表的B和V两色曲线,分别进行了食外测光畸变波的黑子模拟分析,得出WY Cnc在两个时期中,其主子星均存在两个黑子活动区,并给出它们的大小、位置和活动区平均温度结果。新的测光质比为q=m2/m1=0.454±0.005。WY Cnc属主序不接双星。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/52768
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
李炎,解兴发,翟迪生,等. WYCnC的四色uvby测光和食外畸变波的黑子模拟[J]. 天体物理学报,1989,9(2):97.
APA 李炎,解兴发,翟迪生,&陈海林.(1989).WYCnC的四色uvby测光和食外畸变波的黑子模拟.天体物理学报,9(2),97.
MLA 李炎,et al."WYCnC的四色uvby测光和食外畸变波的黑子模拟".天体物理学报 9.2(1989):97.
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