Speaker
SHABNAM AGHAYEVA
(GRANDMA)
Description
The results of the study of photometric observation material obtained in June 2021 with a CCD photometer in the 60-cm telescope of the Shamakhi Astrophysics Observatory named N.Tusi of Wolf 134 type WR 134 star are given. Observations of the star WR 134 were made in filter V of the international UBV photometric system and its short-term (approximately one hour) photometric variability was detected. The mean quadratic error assigned to the control star was 0.004. The MaxIm DL software folder was used to process the photometric images of the star under study.
Author
SHABNAM AGHAYEVA
(GRANDMA)
