CYCLE-TO-CYCLE CHANGES IN THE MIRA-TYPE STAR RT CYG
RT Cyg was observed on photographic negatives of the Odessa plate collection. These data were reduced to the visual AFOEV system. The complete data set (n =7154) was studied by using several methods described by Andronov (l997b). 3-rd order trigonometric polynomial fit to the mean light curve corres...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Odessa I. I. Mechnykov National University
2017-08-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/108189 |