{"title":"塞弗特星系和星暴星系远红外辐射的起源(论文摘要)","authors":"H. Mouri","doi":"10.1086/170993","DOIUrl":null,"url":null,"abstract":"To study the origin of far-IR emission in starburst nuclei (SBNs) and active galactic nuclei (AGNs), the 25-60 μm spectral index [α(25, 60)] has been compared with the intensity ratios of [O I] λ6300 to Hα ([O I]/Hα) and H 2 υ=1-0 S(1) 2.12 μm to Brγ [S(1)/Brγ] for 48 galaxies (16 SBNs, 27 AGNs, and five LINERs).","PeriodicalId":85771,"journal":{"name":"The Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku","volume":"21 1","pages":"239-240"},"PeriodicalIF":0.0000,"publicationDate":"1992-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"29","resultStr":"{\"title\":\"Origin of Far-Infrared Emission in Seyfert and Starburst Galaxies(Abstracts of Doctral Dissertations)\",\"authors\":\"H. Mouri\",\"doi\":\"10.1086/170993\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"To study the origin of far-IR emission in starburst nuclei (SBNs) and active galactic nuclei (AGNs), the 25-60 μm spectral index [α(25, 60)] has been compared with the intensity ratios of [O I] λ6300 to Hα ([O I]/Hα) and H 2 υ=1-0 S(1) 2.12 μm to Brγ [S(1)/Brγ] for 48 galaxies (16 SBNs, 27 AGNs, and five LINERs).\",\"PeriodicalId\":85771,\"journal\":{\"name\":\"The Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku\",\"volume\":\"21 1\",\"pages\":\"239-240\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1992-02-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"29\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1086/170993\",\"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 Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1086/170993","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Origin of Far-Infrared Emission in Seyfert and Starburst Galaxies(Abstracts of Doctral Dissertations)
To study the origin of far-IR emission in starburst nuclei (SBNs) and active galactic nuclei (AGNs), the 25-60 μm spectral index [α(25, 60)] has been compared with the intensity ratios of [O I] λ6300 to Hα ([O I]/Hα) and H 2 υ=1-0 S(1) 2.12 μm to Brγ [S(1)/Brγ] for 48 galaxies (16 SBNs, 27 AGNs, and five LINERs).
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