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New light curve solution of V568 Peg and first determination of its fundamental parameters
DOI: 10.48550/arXiv.1812.09020
Bibcode: 2019BlgAJ..31...68K
Kjurkchieva, Diana; Ibryamov, Sunay
We present V, R_c photometric observations of the short-period W UMa star V568 Peg. They allowed us to improve its period. The light curve solution revealed that V568 Peg is an overcontact binary of A subtype with moderate fill-out factor. Its components are K stars which undergo partial eclipses. The mass ratio was estimated by q-search analysis.…
2019
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Bulgarian Astronomical Journal
Gaia
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