The ISO-SWS survey of molecular hydrogen lines in active galaxies
We present a survey of molecular hydrogen line emission in nearby starburst and Seyfert galaxies. Excitation temperatures and gas masses for loci-lying energy levels of Hz are derived from the observed pure rotational lines. The H-2 (0-0) S(1) line in Seyferts is emitted by a "warm" gas at...
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| Formato: | Conference item |
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1999
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