亮algol型半分离紧密双星系统HU Tauri (HR 1471)的光谱学

Q4 Physics and Astronomy

Information Bulletin on Variable Stars Pub Date : 2017-07-20 DOI:10.22444/IBVS.6233

M. Parthasarathy

{"title":"亮algol型半分离紧密双星系统HU Tauri (HR 1471)的光谱学","authors":"M. Parthasarathy","doi":"10.22444/IBVS.6233","DOIUrl":null,"url":null,"abstract":"Spectroscopic results of HU Tauri that I presented in my Ph.D thesis (Parthasarathy 1979) are published in this paper. The H-alpha line of the secondary is detected. The detection of H-alpha line of the secondary is confirmed based on the high resolution Coude Reticon spectra obtained with the 2.1-m telescope of the McDonald observatory.","PeriodicalId":35213,"journal":{"name":"Information Bulletin on Variable Stars","volume":" ","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2017-07-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Spectroscopy of bright Algol-type semi-detached close binary system HU Tauri (HR 1471)\",\"authors\":\"M. Parthasarathy\",\"doi\":\"10.22444/IBVS.6233\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Spectroscopic results of HU Tauri that I presented in my Ph.D thesis (Parthasarathy 1979) are published in this paper. The H-alpha line of the secondary is detected. The detection of H-alpha line of the secondary is confirmed based on the high resolution Coude Reticon spectra obtained with the 2.1-m telescope of the McDonald observatory.\",\"PeriodicalId\":35213,\"journal\":{\"name\":\"Information Bulletin on Variable Stars\",\"volume\":\" \",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2017-07-20\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Information Bulletin on Variable Stars\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.22444/IBVS.6233\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Information Bulletin on Variable Stars","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22444/IBVS.6233","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}

引用次数: 0

摘要

本文发表了我在1979年发表的博士论文（Parthasarathy）中对胡的光谱结果。检测到次级的H-alpha线。根据麦克唐纳天文台2.1米望远镜获得的高分辨率Coude Reticon光谱，证实了次级的H-alpha线的探测。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

查看原文本刊更多论文

Spectroscopy of bright Algol-type semi-detached close binary system HU Tauri (HR 1471)

Spectroscopic results of HU Tauri that I presented in my Ph.D thesis (Parthasarathy 1979) are published in this paper. The H-alpha line of the secondary is detected. The detection of H-alpha line of the secondary is confirmed based on the high resolution Coude Reticon spectra obtained with the 2.1-m telescope of the McDonald observatory.

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

Information Bulletin on Variable Stars Physics and Astronomy-Astronomy and Astrophysics

CiteScore

0.40

自引率

0.00%

发文量

审稿时长

3 weeks