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The New Photometric Study of a Possible Three-body System AV CMi

Název česky Nová fotometrická studie možného třítělesového systému AV CMi
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LIŠKA Jiří ZEJDA Miloslav LOMOZ František KUČÁKOVÁ Hana JANÍK Jan PODDANÝ Stanislav BRÁT Luboš ŠMELCER Ladislav SVOBODA Petr UHLÁŘ Robert TRNKA Jaroslav CHRASTINA Marek

Rok publikování 2013
Druh Článek v odborném periodiku
Časopis / Zdroj Central European Astrophysical Bulletin
Fakulta / Pracoviště MU

Přírodovědecká fakulta

Citace
www http://adsabs.harvard.edu/abs/2013CEAB...37..201L
Obor Astronomie a nebeská mechanika, astrofyzika
Klíčová slova CCD;photometry;variable star;eclipsing binary;three-body system
Popis We present new results based on the photometric study of an eclipsing object AV CMi. Liakos and Niarchos (2010) obtained preliminary parameters of the system from photometric measurements and discovered a possible low-mass third body which they placed on an unusual inner orbit around one of the binary components. We confirmed depressions in the light curve and analysed observed changes in the whole light curve. The third body system explanation was tested, but we suggest a new, more realistic, alternative interpretation: a blend of two eclipsing binaries with periods of 2.277751 d and 1.03843 d. Astrometric measurements of the centroid position unfortunately yield no evidence about their angular separation.
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