塞弗特星系和星暴星系远红外辐射的起源(论文摘要)

The Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku Pub Date : 1992-02-01 DOI:10.1086/170993

H. Mouri

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引用次数: 29

摘要

为了研究星暴核(SBNs)和活动星系核(AGNs)远红外辐射的来源，对48个星系(16个SBNs, 27个AGNs和5个LINERs)的25-60 μm光谱指数[α(25,60)]与[O I] λ6300 /Hα ([O I]/Hα)和h2 υ=1-0 S(1) 2.12 μm /Brγ [S(1)/Brγ]的强度比进行了比较。

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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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The Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku

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