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V1010 Oph investigated by a cm-class telescope
Zejda, M1; Mikulasek, Z1,2; Zhu LY(朱俐颖)3,4; Qian SB(钱声帮)3,4; Liska, J1; Janik, J1; Zejda, M (reprint author), Masaryk Univ, Dept Theoret Phys & Astrophys, Kotlarska 2, CZ-61137 Brno, Czech Republic.
会议录名称CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO
2014-03
卷号43
期号3
页码462-464
产权排序第3完成单位
收录类别SCI ; CPCI
会议名称Workshop on Observing Techniques, Instrumentation and Science for Metre-Class Telescopes
会议日期2013-09-23
会议地点Stara Lesna, SLOVAKIA
摘要V1010 Oph is a relatively bright near contact binary. We present a new study including four-colour photometry and a model of the system. The uniqueness of our study is in the using of only a centimetre-class telescope with a CCD camera. We show that such small, cheap equipment seems to be very helpful in the investigation of bright variable stars.
语种英语
学科领域Astronomy & Astrophysics
出版者SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST
出版地SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, TATRANSKA LOMINICA, SK-059 60, SLOVAKIA
ISSN号1335-1842
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WOS记录号WOS:000338483100066
WOS研究方向onomy & Astrophysics
WOS类目onomy & Astrophysics
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文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5965
专题双星与变星研究组
中国科学院天体结构与演化重点实验室
通讯作者Zejda, M (reprint author), Masaryk Univ, Dept Theoret Phys & Astrophys, Kotlarska 2, CZ-61137 Brno, Czech Republic.
作者单位1.Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Kotl´aˇrsk´a 2, CZ-611 37 Brno, Czech Republic,
2.Observatory and Planetarium of Johann Palisa, VˇSB–Technical University, Ostrava, Czech Republic
3.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, China
4.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, China
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Zejda, M,Mikulasek, Z,Zhu LY,et al. V1010 Oph investigated by a cm-class telescope[C]. SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, TATRANSKA LOMINICA, SK-059 60, SLOVAKIA:SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST,2014:462-464.
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