ZEJDA, Miloslav, Zdeněk MIKULÁŠEK, Liying ZHU, Shengbang QIAN and Jiří LIŠKA. The Photometric Study of Neglected Short-Period Eclipsing Binary BS Vulpeculae. In Richards, MT Hubeny, I. FROM INTERACTING BINARIES TO EXOPLANETS: ESSENTIAL MODELING TOOLS. CAMBRIDGE: CAMBRIDGE UNIV PRESS, 2012, p. 83-84. ISBN 978-1-107-01982-9. Available from: https://dx.doi.org/10.1017/S1743921311027001.
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Basic information
Original name The Photometric Study of Neglected Short-Period Eclipsing Binary BS Vulpeculae
Authors ZEJDA, Miloslav (203 Czech Republic, guarantor, belonging to the institution), Zdeněk MIKULÁŠEK (203 Czech Republic, belonging to the institution), Liying ZHU (156 China), Shengbang QIAN (156 China) and Jiří LIŠKA (203 Czech Republic, belonging to the institution).
Edition CAMBRIDGE, FROM INTERACTING BINARIES TO EXOPLANETS: ESSENTIAL MODELING TOOLS, p. 83-84, 2 pp. 2012.
Publisher CAMBRIDGE UNIV PRESS
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
RIV identification code RIV/00216224:14310/12:00057150
Organization unit Faculty of Science
ISBN 978-1-107-01982-9
ISSN 1743-9213
Doi http://dx.doi.org/10.1017/S1743921311027001
UT WoS 000309244400024
Keywords in English stars: binaries: eclipsing; stars: fundamental parameters; stars: individual BS Vul
Tags AKR, rivok
Tags International impact, Reviewed
Changed by Changed by: doc. RNDr. Miloslav Zejda, Ph.D., učo 169695. Changed: 10/2/2013 21:28.
Abstract
The preliminary results of a study of a neglected, relatively bright, short-periodic (P=0.48 d), near contact eclipsing binary BS Vulpeculae is given. We present our new complete (BVRI) light curves, and physical parameters of the system based on them, derived by the 2003 version of the Wilson-Van Hamme code.
Links
GA205/08/0003, research and development projectName: Předpovědi rychlosti ztráty hmoty horkých hvězd
Investor: Czech Science Foundation, Mass-loss rate predictions for hot stars
IAA301630901, research and development projectName: Rozložení energie ve spektru horkých hvězd a jeho proměnnost
Investor: Academy of Sciences of the Czech Republic, Spectral energy distribution of hot stars and its variability
ME10099, research and development projectName: Fotometrický výzkum vybraných zákrytových dvojhvězd
Investor: Ministry of Education, Youth and Sports of the CR, Research and Development Programme KONTAKT (ME)
MUNI/A/0968/2009, interní kód MUName: Fyzika hvězd a hvězdných soustav (Acronym: FYHA)
Investor: Masaryk University, Category A
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