LIŠKA, Jiří, Miloslav ZEJDA, František LOMOZ, Hana KUČÁKOVÁ, Jan JANÍK, Stanislav PODDANÝ, Luboš BRÁT, Ladislav ŠMELCER, Petr SVOBODA, Rudolf UHLÁŘ and Jaroslav TRNKA. AV CMi preliminary results from photometric study. Open European Journal on Variable Stars. 2012, vol. 2012, No 0154, p. 4-9. ISSN 1801-5964.
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Basic information
Original name AV CMi preliminary results from photometric study
Authors LIŠKA, Jiří (203 Czech Republic, guarantor, belonging to the institution), Miloslav ZEJDA (203 Czech Republic, belonging to the institution), František LOMOZ (203 Czech Republic), Hana KUČÁKOVÁ (203 Czech Republic), Jan JANÍK (203 Czech Republic, belonging to the institution), Stanislav PODDANÝ (203 Czech Republic), Luboš BRÁT (203 Czech Republic), Ladislav ŠMELCER (203 Czech Republic), Petr SVOBODA (203 Czech Republic), Rudolf UHLÁŘ (203 Czech Republic) and Jaroslav TRNKA (203 Czech Republic).
Edition Open European Journal on Variable Stars, 2012, 1801-5964.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Czech Republic
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/00216224:14310/12:00058304
Organization unit Faculty of Science
Keywords in English stars: binaries: eclipsing; stars: third body; stars: individual AV CMi
Tags AKR, rivok
Tags International impact
Changed by Changed by: doc. RNDr. Miloslav Zejda, Ph.D., učo 169695. Changed: 30/1/2013 11:09.
Abstract
Preliminary results of one year photometric study of eclipsing binary system AV CMi are presented. Possible low-mass third body on unusual orbit in this system was discovered by Liakos & Niarchos (2010). Our measurements confirmed observed dips of brightness in the light curve called transit of third body. Two measurements were used for identification of host star but neither allows convincing decision. The results are contradictory and thus are opposed of three-body system. Blend of two eclipsing systems in the same position on the sky was proposed for this reason. Accuracy of our astrometric measurements did not allowed to detect an awaited shift in position of centroid during eclipse.
Links
GD205/08/H005, research and development projectName: Fyzika Slunce, hvězd a hvězdných soustav
Investor: Czech Science Foundation, Physics of Sun, stars, and stellar systems
MUNI/A/0968/2009, interní kód MUName: Fyzika hvězd a hvězdných soustav (Acronym: FYHA)
Investor: Masaryk University, Category A
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