高重力蓝色大振幅脉冲星 ZTF J071329.02-152125.2 的多周期性

IF 4.5 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Publications of the Astronomical Society of Australia Pub Date : 2024-01-23 DOI:10.1017/pasa.2024.5
Chris Koen
{"title":"高重力蓝色大振幅脉冲星 ZTF J071329.02-152125.2 的多周期性","authors":"Chris Koen","doi":"10.1017/pasa.2024.5","DOIUrl":null,"url":null,"abstract":"New time series photometry of the pulsating hot subdwarf star ZTF J071329.02-152125.2 is presented. Rapid (timescale of hours) changes in the amplitude of the known pulsation in the star was observed. This could be ascribed to beating between three closely spaced frequencies, but analysis of all available photometry finds a range of different frequencies, with widely different amplitudes. A new frequency of 49.66 d<jats:sup>−1</jats:sup>, suggestive of gravity-mode pulsation, was also discovered. The star may be a hybrid p-mode/g-mode hot subdwarf pulsator which sometimes exhibits extraordinarily large amplitude variability.","PeriodicalId":20753,"journal":{"name":"Publications of the Astronomical Society of Australia","volume":"252 1","pages":""},"PeriodicalIF":4.5000,"publicationDate":"2024-01-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Multi-periodicity in the High Gravity Blue Large Amplitude Pulsator ZTF J071329.02-152125.2\",\"authors\":\"Chris Koen\",\"doi\":\"10.1017/pasa.2024.5\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"New time series photometry of the pulsating hot subdwarf star ZTF J071329.02-152125.2 is presented. Rapid (timescale of hours) changes in the amplitude of the known pulsation in the star was observed. This could be ascribed to beating between three closely spaced frequencies, but analysis of all available photometry finds a range of different frequencies, with widely different amplitudes. A new frequency of 49.66 d<jats:sup>−1</jats:sup>, suggestive of gravity-mode pulsation, was also discovered. The star may be a hybrid p-mode/g-mode hot subdwarf pulsator which sometimes exhibits extraordinarily large amplitude variability.\",\"PeriodicalId\":20753,\"journal\":{\"name\":\"Publications of the Astronomical Society of Australia\",\"volume\":\"252 1\",\"pages\":\"\"},\"PeriodicalIF\":4.5000,\"publicationDate\":\"2024-01-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Publications of the Astronomical Society of Australia\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1017/pasa.2024.5\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Publications of the Astronomical Society of Australia","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1017/pasa.2024.5","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

本文介绍了脉动热亚矮星 ZTF J071329.02-152125.2 的新时间序列光度测量。观测到该恒星已知脉动的振幅发生了快速变化(时间尺度为数小时)。这可以归因于三个间隔很近的频率之间的跳动,但对所有可用光度测量的分析却发现了一系列不同的频率,其振幅也相差很大。此外,还发现了一个 49.66 d-1 的新频率,表明这是重力模式脉动。这颗恒星可能是一个混合 p 模式/g 模式的热亚矮脉冲星,有时会表现出非常大的振幅变化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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
Multi-periodicity in the High Gravity Blue Large Amplitude Pulsator ZTF J071329.02-152125.2
New time series photometry of the pulsating hot subdwarf star ZTF J071329.02-152125.2 is presented. Rapid (timescale of hours) changes in the amplitude of the known pulsation in the star was observed. This could be ascribed to beating between three closely spaced frequencies, but analysis of all available photometry finds a range of different frequencies, with widely different amplitudes. A new frequency of 49.66 d−1, suggestive of gravity-mode pulsation, was also discovered. The star may be a hybrid p-mode/g-mode hot subdwarf pulsator which sometimes exhibits extraordinarily large amplitude variability.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia 地学天文-天文与天体物理
CiteScore
5.90
自引率
9.50%
发文量
41
审稿时长
>12 weeks
期刊介绍: Publications of the Astronomical Society of Australia (PASA) publishes new and significant research in astronomy and astrophysics. PASA covers a wide range of topics within astronomy, including multi-wavelength observations, theoretical modelling, computational astronomy and visualisation. PASA also maintains its heritage of publishing results on southern hemisphere astronomy and on astronomy with Australian facilities. PASA publishes research papers, review papers and special series on topical issues, making use of expert international reviewers and an experienced Editorial Board. As an electronic-only journal, PASA publishes paper by paper, ensuring a rapid publication rate. There are no page charges. PASA''s Editorial Board approve a certain number of papers per year to be published Open Access without a publication fee.
期刊最新文献
Increasing the detectability of long-period and nulling pulsars in next-generation pulsar surveys Multi-band optical variability on diverse timescales of blazar 1E 1458.8+2249 Measuring the stellar and planetary parameters of the 51 Eridani system Imaging pulsar census of the galactic plane using MWA VCS data High-time resolution GPU imager for FRB searches at low radio frequencies
×
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