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[vsnet-const 13] V351 Cyg



V351 Cyg

CST star recently studied by Schmidt (1996). According to
his paper, star exhibits eclipses with period 0.104292 d.
But these eclipses were visible only V band, in R band star
showed only scatter (larger than average in stars of its
magnitude). As far as I know no one has studied this star
after Schmidt.

Best regards

Ondrej Pejcha

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