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...
المؤلفون الرئيسيون: | Kunze, D, Rigopoulou, D, Genzel, R, Lutz, D |
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التنسيق: | Conference item |
منشور في: |
1999
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مواد مشابهة
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An ISO-SWS survey of molecular hydrogen in starburst and Seyfert galaxies
حسب: Rigopoulou, D, وآخرون
منشور في: (2002) -
ISO-SWS spectroscopy of Arp 220: A highly obscured starburst galaxy
حسب: Sturm, E, وآخرون
منشور في: (1996) -
SWS spectroscopy of the colliding galaxies NGC 4038/39
حسب: Kunze, D, وآخرون
منشور في: (1996) -
SWS spectroscopy of the starburst galaxy NGC 3256
حسب: Rigopoulou, D, وآخرون
منشور في: (1996) -
ISO spectroscopy of nearby starburst galaxies
حسب: Kunze, D, وآخرون
منشور في: (1999)