ISO spectroscopy of nearby starburst galaxies
We present spectroscopic mid-IR observations of prominent starburst galaxies obtained with the short wavelength spectrometer onboard the Infrared Space Observatory. The wavelength range accessible by ISO-sws (2.5-45 pm) contains a large number of emission lines of atomic and molecular hydrogen and s...
| Autores principales: | , , , , |
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| Formato: | Conference item |
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1999
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| _version_ | 1826270420531150848 |
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| author | Kunze, D Lutz, D Rigopoulou, D Thornley, MD Genzel, R |
| author_facet | Kunze, D Lutz, D Rigopoulou, D Thornley, MD Genzel, R |
| author_sort | Kunze, D |
| collection | OXFORD |
| description | We present spectroscopic mid-IR observations of prominent starburst galaxies obtained with the short wavelength spectrometer onboard the Infrared Space Observatory. The wavelength range accessible by ISO-sws (2.5-45 pm) contains a large number of emission lines of atomic and molecular hydrogen and several other atomic species. In this paper we discuss the interpretation of the [NeIII] 15.5 mum/[NeII] 12.8 mum line-ratio, the faint [OIV] 25.9 mum line and the pure rotational lines of molecular hydrogen observed in our target galaxies. |
| first_indexed | 2024-03-06T21:40:33Z |
| format | Conference item |
| id | oxford-uuid:47c8b25b-6c21-4f6c-8a2f-acb2548fd478 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T21:40:33Z |
| publishDate | 1999 |
| record_format | dspace |
| spelling | oxford-uuid:47c8b25b-6c21-4f6c-8a2f-acb2548fd4782022-03-26T15:21:57ZISO spectroscopy of nearby starburst galaxiesConference itemhttp://purl.org/coar/resource_type/c_5794uuid:47c8b25b-6c21-4f6c-8a2f-acb2548fd478Symplectic Elements at Oxford1999Kunze, DLutz, DRigopoulou, DThornley, MDGenzel, RWe present spectroscopic mid-IR observations of prominent starburst galaxies obtained with the short wavelength spectrometer onboard the Infrared Space Observatory. The wavelength range accessible by ISO-sws (2.5-45 pm) contains a large number of emission lines of atomic and molecular hydrogen and several other atomic species. In this paper we discuss the interpretation of the [NeIII] 15.5 mum/[NeII] 12.8 mum line-ratio, the faint [OIV] 25.9 mum line and the pure rotational lines of molecular hydrogen observed in our target galaxies. |
| spellingShingle | Kunze, D Lutz, D Rigopoulou, D Thornley, MD Genzel, R ISO spectroscopy of nearby starburst galaxies |
| title | ISO spectroscopy of nearby starburst galaxies |
| title_full | ISO spectroscopy of nearby starburst galaxies |
| title_fullStr | ISO spectroscopy of nearby starburst galaxies |
| title_full_unstemmed | ISO spectroscopy of nearby starburst galaxies |
| title_short | ISO spectroscopy of nearby starburst galaxies |
| title_sort | iso spectroscopy of nearby starburst galaxies |
| work_keys_str_mv | AT kunzed isospectroscopyofnearbystarburstgalaxies AT lutzd isospectroscopyofnearbystarburstgalaxies AT rigopouloud isospectroscopyofnearbystarburstgalaxies AT thornleymd isospectroscopyofnearbystarburstgalaxies AT genzelr isospectroscopyofnearbystarburstgalaxies |