wuma型系统的二维参数关系

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Atila Poro, Ehsan Paki, Ailar Alizadehsabegh, Mehdi Khodadadilori, Selda Ranjbar Salehian, Mahya Hedayatjoo, Fatemeh Hashemi, Yasaman Dashti, Fatemeh Mohammadizadeh
{"title":"wuma型系统的二维参数关系","authors":"Atila Poro, Ehsan Paki, Ailar Alizadehsabegh, Mehdi Khodadadilori, Selda Ranjbar Salehian, Mahya Hedayatjoo, Fatemeh Hashemi, Yasaman Dashti, Fatemeh Mohammadizadeh","doi":"10.1088/1674-4527/ad0866","DOIUrl":null,"url":null,"abstract":"Abstract Reviewing the empirical and theoretical parameter relationships between various parameters is a good way to understand more about contact binary systems. In this investigation, two-dimensional (2D) relationships for $P-M_{V(system)}$, $P-L_{1,2}$, $M_{1,2}-L_{1,2}$, and $q-L_{ratio}$ were revisited. The sample used is related to 118 contact binary systems with an orbital period shorter than 0.6 days whose absolute parameters were estimated based on the $Gaia$ Data Release 3 (DR3) parallax. We reviewed previous studies on 2D relationships and updated six parameter relationships. Therefore, Markov chain Monte Carlo (MCMC) and machine learning methods were used, and the outcomes were compared. We selected 22 contact binary systems from eight previous studies for comparison, which had light curve solutions using spectroscopic data. The results show that the systems are in good agreement with the results of this study.","PeriodicalId":54494,"journal":{"name":"Research in Astronomy and Astrophysics","volume":"67 1 1","pages":"0"},"PeriodicalIF":1.8000,"publicationDate":"2023-10-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Two-dimensional Parameter Relationships for W UMa-type Systems Revisited\",\"authors\":\"Atila Poro, Ehsan Paki, Ailar Alizadehsabegh, Mehdi Khodadadilori, Selda Ranjbar Salehian, Mahya Hedayatjoo, Fatemeh Hashemi, Yasaman Dashti, Fatemeh Mohammadizadeh\",\"doi\":\"10.1088/1674-4527/ad0866\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Abstract Reviewing the empirical and theoretical parameter relationships between various parameters is a good way to understand more about contact binary systems. In this investigation, two-dimensional (2D) relationships for $P-M_{V(system)}$, $P-L_{1,2}$, $M_{1,2}-L_{1,2}$, and $q-L_{ratio}$ were revisited. The sample used is related to 118 contact binary systems with an orbital period shorter than 0.6 days whose absolute parameters were estimated based on the $Gaia$ Data Release 3 (DR3) parallax. We reviewed previous studies on 2D relationships and updated six parameter relationships. Therefore, Markov chain Monte Carlo (MCMC) and machine learning methods were used, and the outcomes were compared. We selected 22 contact binary systems from eight previous studies for comparison, which had light curve solutions using spectroscopic data. The results show that the systems are in good agreement with the results of this study.\",\"PeriodicalId\":54494,\"journal\":{\"name\":\"Research in Astronomy and Astrophysics\",\"volume\":\"67 1 1\",\"pages\":\"0\"},\"PeriodicalIF\":1.8000,\"publicationDate\":\"2023-10-31\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Research in Astronomy and Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1088/1674-4527/ad0866\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research in Astronomy and Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1088/1674-4527/ad0866","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

回顾各种参数之间的经验和理论参数关系是更好地理解接触二元系统的好方法。在本研究中,重新研究了$P-M_{V(system)}$、$P-L_{1,2}$、$M_{1,2} $和$q-L_{ratio}$的二维(2D)关系。所使用的样本与118个接触双星系统有关,它们的轨道周期小于0.6天,其绝对参数是根据$Gaia$数据发布3 (DR3)视差估计的。我们回顾了以往关于二维关系的研究,并更新了六个参数关系。因此,使用了马尔可夫链蒙特卡罗(MCMC)和机器学习方法,并比较了结果。我们从先前的8个研究中选择了22个接触双星系统进行比较,这些系统使用光谱数据获得了光曲线解。结果表明,该系统与本研究结果吻合较好。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Two-dimensional Parameter Relationships for W UMa-type Systems Revisited
Abstract Reviewing the empirical and theoretical parameter relationships between various parameters is a good way to understand more about contact binary systems. In this investigation, two-dimensional (2D) relationships for $P-M_{V(system)}$, $P-L_{1,2}$, $M_{1,2}-L_{1,2}$, and $q-L_{ratio}$ were revisited. The sample used is related to 118 contact binary systems with an orbital period shorter than 0.6 days whose absolute parameters were estimated based on the $Gaia$ Data Release 3 (DR3) parallax. We reviewed previous studies on 2D relationships and updated six parameter relationships. Therefore, Markov chain Monte Carlo (MCMC) and machine learning methods were used, and the outcomes were compared. We selected 22 contact binary systems from eight previous studies for comparison, which had light curve solutions using spectroscopic data. The results show that the systems are in good agreement with the results of this study.
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
Research in Astronomy and Astrophysics
Research in Astronomy and Astrophysics 地学天文-天文与天体物理
CiteScore
3.20
自引率
16.70%
发文量
2599
审稿时长
6.0 months
期刊介绍: Research in Astronomy and Astrophysics (RAA) is an international journal publishing original research papers and reviews across all branches of astronomy and astrophysics, with a particular interest in the following topics: -large-scale structure of universe formation and evolution of galaxies- high-energy and cataclysmic processes in astrophysics- formation and evolution of stars- astrogeodynamics- solar magnetic activity and heliogeospace environments- dynamics of celestial bodies in the solar system and artificial bodies- space observation and exploration- new astronomical techniques and methods
×
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
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
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 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信