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Multicolor study of V1009 Per, a close binary system at the beginning of the overcontact phase, and of CRTS J031642.2+332639, a new binary system in the same field

The first multicolor observations and light curve solutions of the eclipsing binary systems V1009 Per and CRTS J031642.2+332639 are presented. Using the 2005 version of the Wilson-Devinney code, both systems are found to be W UMa contact binaries. V1009 Per has a mass ratio of q = 0.362 ± 0.002 and...

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Pubblicato in:Revista Mexicana de Astronomía y Astrofísica
Autori principali: Raúl Michel, Francesco Acerbi, Carlo Barani, Massimiliano Martignoni
Natura: Artigo
Lingua:Inglês
Pubblicazione: Universidad Nacional Autónoma de México 2019
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Accesso online:https://www.redalyc.org/articulo.oa?id=57171616008
https://www.redalyc.org/journal/571/57171616008/
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https://www.redalyc.org/journal/571/57171616008/57171616008.epub
https://www.redalyc.org/journal/571/57171616008/movil
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