UBV Light Curves of ζ AUR Star 32 Cygni

UBV Light Curves of ζ AUR Star 32 Cygni

UBV ovservation of ζ Aur star 32 Cyg have been at the Yonsei University Observatory suing the 60-cm Goto reflector and five years, 1988-1992. Observations made during these years cover outside of eclipse phase only. No significant light variation which would represent the secondary eclipse of red su...

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Bibliographic Details
Main Authors:	Il-Seong Nha, Yonggi Kim, Yong-Sam lee
Format:	Article
Language:	English
Published:	The Korean Space Science Society 1992-12-01
Series:	Journal of Astronomy and Space Sciences
Online Access:	http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n2/OJOOBS_1992_v9n2_127.pdf

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