斯库蒂三角洲变星2MASS J13122513+5443409的UMa光度研究

A. Maliuk, V. Krushevska, S. Shugarov, Z. Garai, Ya. Romanyuk, Y. Kuznyetsova, M. Andreev
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引用次数: 0

摘要

.我们继续研究我们小组之前发现的德尔塔苏蒂型 2MASS J13122513+5443409 新变星。我们不仅分析了从斯洛伐克和乌克兰相对较小的望远镜中获得的数据,还分析了从 TESS 任务中获得的数据。我们利用 Lomb-Scargle 周期图计算了脉动周期和振幅。我们发现主周期约为 0 .079 天。然而,振荡显示出跳动,表明存在多个脉冲频率。
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Photometric study of the Delta Scuti variable 2MASS J13122513+5443409 in UMa
. We keep investigating the new variable of Delta Scuti type 2MASS J13122513+5443409 discovered by our group previously. We have analyzed the data obtained not only from the relatively small telescopes of Slovakia and Ukraine, but also from the TESS mission. We calculated the pulsation period and amplitude using the Lomb-Scargle periodogram. We found that the dominant period is about 0 . 079 days. However, the oscillations displayed beating, indicating the presence of several pulsation frequencies.
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