{"title":"选定行星状星云中心恒星温度的测定","authors":"A. H. Alili, K. Alisheva, Kh. M. Mikailov","doi":"10.18524/1810-4215.2023.36.290929","DOIUrl":null,"url":null,"abstract":"In this work, for planetary nebulae İC 1295, İC 4191, Zanstra temperatures were calculated using the Hβ line of the central stars. Respectively, the temperatures 64252 K and 47663 K were determined. The flux in the Hβ radiative line used in the calculations, has been determined from the spectra retrieved from the archive of the European Southern Observatory. Our results have been compared with results of the other authors.","PeriodicalId":34039,"journal":{"name":"Odessa Astronomical Publications","volume":"328 ","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2023-12-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"DETERMINATION OF THE TEMPERATURES OF THE CENTRAL STARS OF SELECTED PLANETARY NEBULAE\",\"authors\":\"A. H. Alili, K. Alisheva, Kh. M. Mikailov\",\"doi\":\"10.18524/1810-4215.2023.36.290929\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this work, for planetary nebulae İC 1295, İC 4191, Zanstra temperatures were calculated using the Hβ line of the central stars. Respectively, the temperatures 64252 K and 47663 K were determined. The flux in the Hβ radiative line used in the calculations, has been determined from the spectra retrieved from the archive of the European Southern Observatory. Our results have been compared with results of the other authors.\",\"PeriodicalId\":34039,\"journal\":{\"name\":\"Odessa Astronomical Publications\",\"volume\":\"328 \",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-12-04\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Odessa Astronomical Publications\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.18524/1810-4215.2023.36.290929\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Odessa Astronomical Publications","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.18524/1810-4215.2023.36.290929","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
在这项工作中，利用中心恒星的Hβ线计算了行星状星云İC 1295和İC 4191的赞斯特拉温度。分别测定了 64252 K 和 47663 K 的温度。计算中使用的 Hβ 辐射线的通量是根据从欧洲南方天文台档案中获取的光谱确定的。我们的结果与其他作者的结果进行了比较。
DETERMINATION OF THE TEMPERATURES OF THE CENTRAL STARS OF SELECTED PLANETARY NEBULAE
In this work, for planetary nebulae İC 1295, İC 4191, Zanstra temperatures were calculated using the Hβ line of the central stars. Respectively, the temperatures 64252 K and 47663 K were determined. The flux in the Hβ radiative line used in the calculations, has been determined from the spectra retrieved from the archive of the European Southern Observatory. Our results have been compared with results of the other authors.
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