Polaris: History of Pulsation Activity since Discovery

I. O. Usenko, V. Kovtyukh, A. Miroshnichenko, S. Danford
{"title":"Polaris: History of Pulsation Activity since Discovery","authors":"I. O. Usenko, V. Kovtyukh, A. Miroshnichenko, S. Danford","doi":"10.15407/SCIN13.01.109","DOIUrl":null,"url":null,"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.","PeriodicalId":19061,"journal":{"name":"Nauka ta Innovacii","volume":"13 1","pages":"109-113"},"PeriodicalIF":0.0000,"publicationDate":"2017-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nauka ta Innovacii","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.15407/SCIN13.01.109","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
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.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
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。
求助全文
约1分钟内获得全文 去求助
来源期刊
自引率
0.00%
发文量
0
审稿时长
12 weeks
期刊最新文献
Internal student migration in India: Impact of the COVID-19 crisis. Fiscal Regulation of National Economies' Sustainable Growth Research of Possibility of Control of the Formation of Crystal structure of Metal Alloys System Cryogenic Supply Cryomagnetic Complex KMK–1000 on the Basis of Micro-Cryogenic Systems of Closed Cicle Phytomodule Cluster as a Structural Element of Indoor Area of Various Functional Purpose
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1