Be星LQ And和EM Cep的快速光变 |
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引用本文: | 杭恒荣,黄磷.Be星LQ And和EM Cep的快速光变[J].紫金山天文台台刊,1994,13(1):76. |
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作者姓名: | 杭恒荣 黄磷 |
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摘 要: | UBV photometric observations of LQ And and EM Cep were made with 60 cm telescope at Beijing Astronomical Observatory from 1990 to 1992. Some results are briefly summarized as follows:(1) LQ And317 data sets have been obtained. HR9011 was used as the comparison star. Combining these data with some published VBV measurements of secured during 1983-1988, an improved period of light variation has been derived, and a new ephemeris for minimum light has been suggested:T min. light = HJD 2445621.5964 0.309418 × E.(2) EM Cep277 data sets have been obtained. HD208218 was used as the comparison star. With these data a minimum light time base been derived at HJD 2448912.0452. Combining this value with all published previously, an improved linear ephemeris has been derived with a rms of 0.01382:T min. light = HJD 2440134.7338 0.8061840 x EIt is of interest to note that there is also a possibility of decrease tendency of the period. We have derived an ephemeris by using a binomial fitting with a rms of 0.01155:
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关 键 词: | Be星 LQAnd EMCep 光变 |
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