IMPROVED EPHEMERIS OF POORLY STUDIED ECLIPSING BINARY GSC 3950-00707 = 2MASS J20355082+5242136
Journal Title: Odessa Astronomical Publications - Year 2017, Vol 30, Issue
Abstract
We made our CCD-observations of GSC 3950-00707 by using the telescope Celestron-14 of Vihorlat Observatory and Astronomical Observatory on Kolonica Saddle. The moments of minima were calculated by using the symmetrical polynomial fit. We also analyzed the observations from automated surveys ASAS-SN and found 3 mean minima by using trigonometrical polynomial fit. The analysis of our observations and data from the surveys allows to conclude that it is the W UMa-type variable and its published period value is not accurate. We analyzed the O-C curve and corrected the elements.
Authors and Affiliations
S. V. Savastru, V. I. Marsakova, K. D. Andrych, P. Dubovsky
Keywords
Related Articles
- EP ID EP349371
- DOI 10.18524/1810-4215.2017.30.115819
- Views 85
- Downloads 0
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