{"title":"恒星大气","authors":"K. Werner","doi":"10.1142/9781783265817_0005","DOIUrl":null,"url":null,"abstract":"We summarize recent eeorts in non-LTE modeling of stellar atmospheres. We outline the basic idea of the Accelerated Lambda Iteration method and further improvements in numerical techniques which nally lead to metal line blanketed NLTE models. Some applications of the new models are highlighted.","PeriodicalId":399070,"journal":{"name":"The Structure and Evolution of Stars","volume":"28 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2019-01-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Stellar Atmospheres\",\"authors\":\"K. Werner\",\"doi\":\"10.1142/9781783265817_0005\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We summarize recent eeorts in non-LTE modeling of stellar atmospheres. We outline the basic idea of the Accelerated Lambda Iteration method and further improvements in numerical techniques which nally lead to metal line blanketed NLTE models. Some applications of the new models are highlighted.\",\"PeriodicalId\":399070,\"journal\":{\"name\":\"The Structure and Evolution of Stars\",\"volume\":\"28 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2019-01-07\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The Structure and Evolution of Stars\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1142/9781783265817_0005\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"The Structure and Evolution of Stars","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1142/9781783265817_0005","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
We summarize recent eeorts in non-LTE modeling of stellar atmospheres. We outline the basic idea of the Accelerated Lambda Iteration method and further improvements in numerical techniques which nally lead to metal line blanketed NLTE models. Some applications of the new models are highlighted.
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