来自盖亚DR3和JWST数据的猎户座星云集群(ONC)和行星系统

IF 0.7 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
S. V. Vereshchagin, D. I. Tagaev, T. Bugra Keskin, N. V. Chupina, E. S. Postnikova
{"title":"来自盖亚DR3和JWST数据的猎户座星云集群(ONC)和行星系统","authors":"S. V. Vereshchagin,&nbsp;D. I. Tagaev,&nbsp;T. Bugra Keskin,&nbsp;N. V. Chupina,&nbsp;E. S. Postnikova","doi":"10.1134/S106377292570163X","DOIUrl":null,"url":null,"abstract":"<p>Using Gaia DR3 data, we studied the Orion Nebula Cluster (ONC) in the region of the sky where free planets and stars with planetary systems were discovered using the James Webb Space Telescope (JWST). We selected ONC candidate stars for which the probabilities of belonging to the cluster were estimated. Using Gaia DR3 star parallaxes, we determined the distance of the ONC from the Sun to be 393 ± 13 pc. The analysis allowed us to estimate the number of single and binary stars, the number of stars with planets, and the number of free planets in the selected region of space in the central part of the ONC. Our estimates indicate the possibility of obtaining new results from numerical modeling.</p>","PeriodicalId":55440,"journal":{"name":"Astronomy Reports","volume":"69 3","pages":"157 - 168"},"PeriodicalIF":0.7000,"publicationDate":"2025-06-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Orion Nebula Cluster (ONC) and Planetary Systems from Gaia DR3 and JWST Data\",\"authors\":\"S. V. Vereshchagin,&nbsp;D. I. Tagaev,&nbsp;T. Bugra Keskin,&nbsp;N. V. Chupina,&nbsp;E. S. Postnikova\",\"doi\":\"10.1134/S106377292570163X\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Using Gaia DR3 data, we studied the Orion Nebula Cluster (ONC) in the region of the sky where free planets and stars with planetary systems were discovered using the James Webb Space Telescope (JWST). We selected ONC candidate stars for which the probabilities of belonging to the cluster were estimated. Using Gaia DR3 star parallaxes, we determined the distance of the ONC from the Sun to be 393 ± 13 pc. The analysis allowed us to estimate the number of single and binary stars, the number of stars with planets, and the number of free planets in the selected region of space in the central part of the ONC. Our estimates indicate the possibility of obtaining new results from numerical modeling.</p>\",\"PeriodicalId\":55440,\"journal\":{\"name\":\"Astronomy Reports\",\"volume\":\"69 3\",\"pages\":\"157 - 168\"},\"PeriodicalIF\":0.7000,\"publicationDate\":\"2025-06-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomy Reports\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S106377292570163X\",\"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":"Astronomy Reports","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S106377292570163X","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

利用盖亚DR3的数据,我们研究了猎户座星云星团(ONC)的天空区域,在那里使用詹姆斯韦伯太空望远镜(JWST)发现了自由行星和具有行星系统的恒星。我们选择了ONC候选恒星,估计了它们属于该星团的概率。利用盖亚DR3恒星的视差,我们确定了ONC与太阳的距离为393±13 pc。分析使我们能够估计出ONC中心选定空间区域内单星和双星的数量,有行星的恒星的数量,以及自由行星的数量。我们的估计表明有可能从数值模拟中获得新的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Orion Nebula Cluster (ONC) and Planetary Systems from Gaia DR3 and JWST Data

Orion Nebula Cluster (ONC) and Planetary Systems from Gaia DR3 and JWST Data

Using Gaia DR3 data, we studied the Orion Nebula Cluster (ONC) in the region of the sky where free planets and stars with planetary systems were discovered using the James Webb Space Telescope (JWST). We selected ONC candidate stars for which the probabilities of belonging to the cluster were estimated. Using Gaia DR3 star parallaxes, we determined the distance of the ONC from the Sun to be 393 ± 13 pc. The analysis allowed us to estimate the number of single and binary stars, the number of stars with planets, and the number of free planets in the selected region of space in the central part of the ONC. Our estimates indicate the possibility of obtaining new results from numerical modeling.

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
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
×
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:604180095
Book学术官方微信