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- W2012174530 abstract "The low-luminosity active nucleus of M51 is shown to be a strong source of emission in the 1-0 S (1) line of H2. The emission appears to be extended on a scale of 200 pc. On the basis of the strength of this line relative to Brackett-gamma, it can be argued that the emission is produced in gas that is shocked, possibly by outflows from this low-luminosity Seyfert-like nucleus. Previously, a large H2 1-0 S(1)/Brackett-gamma ratio was a characteristic seen only in high-luminosity nuclei. 30 refs." @default.
- W2012174530 created "2016-06-24" @default.
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- W2012174530 date "1990-01-01" @default.
- W2012174530 modified "2023-09-27" @default.
- W2012174530 title "Strong molecular hydrogen emission from the low-luminosity nucleus of M51" @default.
- W2012174530 doi "https://doi.org/10.1086/185628" @default.
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