Polaris: History of Pulsation Activity since Discovery

I. O. Usenko, V. Kovtyukh, A. Miroshnichenko, S. Danford
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引用次数: 1

Abstract

The pulsation activity of small-amplitude Cepheid Alpha UMi (Polaris) during the period of its radial velocity observations has been analyzed. In the 20th century, Polaris was known to demonstrate a decrease in radial velocity amplitude to the minimum, in the 1980s. Thereafter, the amplitude has increased. The observations of September-December 2015 (21 spectra) obtained by 81cm telescope TCO with spectrograph have showed that radial velocity amplitude comes to 4.16 km/s and is approximately twice higher than the estimates made in 2007, with pulsation period adding 8.6 min.
北极星:自发现以来脉动活动的历史
分析了小振幅造父变星α UMi(北极星)在径向速度观测期间的脉动活动。在20世纪80年代,北极星的径向速度幅值下降到最小值。此后,振幅有所增加。利用81cm望远镜TCO和摄谱仪获得的2015年9 - 12月(21个光谱)观测结果表明,径向速度幅值达到4.16 km/s,比2007年估计的值提高了约两倍,脉动周期增加了8.6 min。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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