Thayse A. PACHECO, Ronaldo S. LEVENHAGEN, Marcos P. DIAZ, Paula R. T. COELHO
{"title":"非lte线覆盖大气结构的网格和亚矮星的合成光谱","authors":"Thayse A. PACHECO, Ronaldo S. LEVENHAGEN, Marcos P. DIAZ, Paula R. T. COELHO","doi":"10.25518/0037-9565.11238","DOIUrl":null,"url":null,"abstract":"We present an update of the grid of detailed atmosphere models and homogeneous synthetic spectra for hot, high-gravity subdwarf stars. High-resolution spectra and synthetic photometry were calculated in the wavelength range 1,000 Å – 10,000 Å using Non-LTE extensively line-blanketed atmosphere structures.","PeriodicalId":35838,"journal":{"name":"Bulletin de la Societe Royale des Sciences de Liege","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A grid of Non-LTE line-blanketed atmosphere structures and synthetic spectra for subdwarfs\",\"authors\":\"Thayse A. PACHECO, Ronaldo S. LEVENHAGEN, Marcos P. DIAZ, Paula R. T. COELHO\",\"doi\":\"10.25518/0037-9565.11238\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We present an update of the grid of detailed atmosphere models and homogeneous synthetic spectra for hot, high-gravity subdwarf stars. High-resolution spectra and synthetic photometry were calculated in the wavelength range 1,000 Å – 10,000 Å using Non-LTE extensively line-blanketed atmosphere structures.\",\"PeriodicalId\":35838,\"journal\":{\"name\":\"Bulletin de la Societe Royale des Sciences de Liege\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Bulletin de la Societe Royale des Sciences de Liege\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.25518/0037-9565.11238\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"Multidisciplinary\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin de la Societe Royale des Sciences de Liege","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.25518/0037-9565.11238","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"Multidisciplinary","Score":null,"Total":0}
引用次数: 0
摘要
我们提出了热的、高重力的亚矮星的详细大气模型网格和均匀合成光谱的更新。在波长范围为1,000 Å - 10,000 Å的高分辨率光谱和合成光度计算使用非lte广泛线覆盖的大气结构。
A grid of Non-LTE line-blanketed atmosphere structures and synthetic spectra for subdwarfs
We present an update of the grid of detailed atmosphere models and homogeneous synthetic spectra for hot, high-gravity subdwarf stars. High-resolution spectra and synthetic photometry were calculated in the wavelength range 1,000 Å – 10,000 Å using Non-LTE extensively line-blanketed atmosphere structures.
期刊介绍:
The ‘Société Royale des Sciences de Liège" (hereafter the Society) regularly publishes in its ‘Bulletin" original scientific papers in the fields of astrophysics, biochemistry, biophysics, biology, chemistry, geology, mathematics, mineralogy or physics, following peer review approval.