Proper identification of variable star V683 Cas
S. Corsato, C. Di Lauro, G. Gasperi, S. Grasso, I. Innocente, R., Possemato, C. Benna, D. Gardiol, G. Pettiti, R. Nesci
TL;DR
This paper clarifies that the variable star V683 Cas is actually an eclipsing binary system, based on photometric observations and analysis of the star's position and nearby stars.
Contribution
It provides the first detailed photometric observations confirming the true nature of V683 Cas as an eclipsing binary system.
Findings
V683 Cas is an eclipsing binary system GSC 03699-00091.
Photometric data supports the reclassification of V683 Cas.
Nearby stars' observations were also reported.
Abstract
Investigation on the object reported by SIMBAD database as V683 Cas shows that this variable star corresponds to the eclipsing binary system GSC 03699-00091 (also identified as NSVS 1850718). The results of the photometric observations of the stars nearby to the position indicated for V683 Cas are reported.
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation