CCD Photometry of W UMa Type Binary TY UMa

CCD Photometry of W UMa Type Binary TY UMa

We present VRI CCD photometry of W UMa type binary TY UMa. The light curves show that the secondary minimum is deeper than theprimary minimum and the maximum I (0.p25) is 0.m023 brighter than the maximum II (0.p75). The V light curve has beenanalyzed and the photometric solutions have been determine...

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Bibliographic Details
Main Authors: Young Woon Kang, Chang Deok Hwang, Hee-Won Lee, Chun-Hwey Kim
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2001-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
STARS
BINARY STARS
STAR SPOT
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2001/v18n1/OJOOBS_2001_v18n1_55.pdf

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