{"title":"Oxygen Abundances from Infrared OH Lines","authors":"S. Balachandran, J. Carr, B. Carney","doi":"10.1017/S1539299600013964","DOIUrl":null,"url":null,"abstract":"Abstract Oxygen abundances are derived from the vibrational–rotational OH lines in the infrared. The flat trend of [O/Fe] between −2.5","PeriodicalId":422890,"journal":{"name":"Highlights of Astronomy","volume":"34 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2001-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"14","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Highlights of Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1017/S1539299600013964","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 14
Abstract
Abstract Oxygen abundances are derived from the vibrational–rotational OH lines in the infrared. The flat trend of [O/Fe] between −2.5
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