盖亚EDR3三颗年轻恒星的数据

K. Gigoyan, N. Azatyan, K. Gigoyan
{"title":"盖亚EDR3三颗年轻恒星的数据","authors":"K. Gigoyan, N. Azatyan, K. Gigoyan","doi":"10.52526/25792776-22.69.1-77","DOIUrl":null,"url":null,"abstract":"We present Gaia Early Data Release 3 (Gaia EDR3) high accurate astrometric and photometric data\nand also Catalina Sky Survey (CSS ) phase-dependent light curves for three Young Stellar Objects (YSO).\nThey are LRL 245, 2MASS J04300424+3533238, and CVSO 592. These tree YSOs are presented as periodic variables in the Catalina Surveys Data Release-1 (CSDR1) data base.\nCSS phase-dependent curve of LRL 245 shows periodicity with period P=234.66 days and amplitude\n∆m≈4.0 mag. For this object high-resolution spectra in H-band (from 1.51 to 1.69 µm) was obtained by\nthe APOGEE instrument. LAMOST telescope moderate-resolution CCD spectra is available for object\n2MASS J04300424+3522238 only. The spectra shows clear features of M dwarfs.","PeriodicalId":412578,"journal":{"name":"Communications of the Byurakan Astrophysical Observatory","volume":"6 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-09-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Gaia EDR3 Data For Three Young Stellar Objects\",\"authors\":\"K. Gigoyan, N. Azatyan, K. Gigoyan\",\"doi\":\"10.52526/25792776-22.69.1-77\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We present Gaia Early Data Release 3 (Gaia EDR3) high accurate astrometric and photometric data\\nand also Catalina Sky Survey (CSS ) phase-dependent light curves for three Young Stellar Objects (YSO).\\nThey are LRL 245, 2MASS J04300424+3533238, and CVSO 592. These tree YSOs are presented as periodic variables in the Catalina Surveys Data Release-1 (CSDR1) data base.\\nCSS phase-dependent curve of LRL 245 shows periodicity with period P=234.66 days and amplitude\\n∆m≈4.0 mag. For this object high-resolution spectra in H-band (from 1.51 to 1.69 µm) was obtained by\\nthe APOGEE instrument. LAMOST telescope moderate-resolution CCD spectra is available for object\\n2MASS J04300424+3522238 only. The spectra shows clear features of M dwarfs.\",\"PeriodicalId\":412578,\"journal\":{\"name\":\"Communications of the Byurakan Astrophysical Observatory\",\"volume\":\"6 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-09-02\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Communications of the Byurakan Astrophysical Observatory\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.52526/25792776-22.69.1-77\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Communications of the Byurakan Astrophysical Observatory","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.52526/25792776-22.69.1-77","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

摘要

我们提供了盖亚早期数据发布3 (Gaia EDR3)的高精度天文测量和光度数据,以及卡塔利娜巡天(CSS)对三颗年轻恒星天体(YSO)的相位相关光曲线。它们是lrl245, 2MASS J04300424+3533238和CVSO 592。LRL 245的css相位曲线具有周期性,周期P=234.66 d,幅值∆m≈4.0等。通过APOGEE仪器获得了该天体h波段(1.51 ~ 1.69µm)的高分辨率光谱。LAMOST望远镜中分辨率CCD光谱仅适用于object2MASS J04300424+3522238。光谱显示了M矮星的清晰特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Gaia EDR3 Data For Three Young Stellar Objects
We present Gaia Early Data Release 3 (Gaia EDR3) high accurate astrometric and photometric data and also Catalina Sky Survey (CSS ) phase-dependent light curves for three Young Stellar Objects (YSO). They are LRL 245, 2MASS J04300424+3533238, and CVSO 592. These tree YSOs are presented as periodic variables in the Catalina Surveys Data Release-1 (CSDR1) data base. CSS phase-dependent curve of LRL 245 shows periodicity with period P=234.66 days and amplitude ∆m≈4.0 mag. For this object high-resolution spectra in H-band (from 1.51 to 1.69 µm) was obtained by the APOGEE instrument. LAMOST telescope moderate-resolution CCD spectra is available for object 2MASS J04300424+3522238 only. The spectra shows clear features of M dwarfs.
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
自引率
0.00%
发文量
0
×
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