ISO observations of starburst and ultraluminous galaxies
We report first results on Infrared Space Observatory (ISO) spectroscopic observations of Starburst and Ultraluminous Galaxies. Observations of a wide range of ionic, atomic, and molecular infrared lines enable us to explore in detail the physical conditions in the circumnuclear regions of these gal...
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| Fformat: | Conference item |
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1997
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| _version_ | 1826290009284542464 |
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| author | Rigopoulou, D Lutz, D Genzel, R Egami, E Kunze, D Sturm, E |
| author_facet | Rigopoulou, D Lutz, D Genzel, R Egami, E Kunze, D Sturm, E |
| author_sort | Rigopoulou, D |
| collection | OXFORD |
| description | We report first results on Infrared Space Observatory (ISO) spectroscopic observations of Starburst and Ultraluminous Galaxies. Observations of a wide range of ionic, atomic, and molecular infrared lines enable us to explore in detail the physical conditions in the circumnuclear regions of these galaxies, and to determine, as a first step, parameters such as gas densities and temperatures of ionizing stars. With the help of theoretical modeling this multi-line spectroscopic database is used to further probe the central emission mechanism, discriminate between stellar and non-thermal processes and finally constrain the current models of galactic nuclei. |
| first_indexed | 2024-03-07T02:37:37Z |
| format | Conference item |
| id | oxford-uuid:a952fa93-5346-4f5e-ab43-cb6235706862 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T02:37:37Z |
| publishDate | 1997 |
| record_format | dspace |
| spelling | oxford-uuid:a952fa93-5346-4f5e-ab43-cb62357068622022-03-27T03:07:40ZISO observations of starburst and ultraluminous galaxiesConference itemhttp://purl.org/coar/resource_type/c_5794uuid:a952fa93-5346-4f5e-ab43-cb6235706862Symplectic Elements at Oxford1997Rigopoulou, DLutz, DGenzel, REgami, EKunze, DSturm, EWe report first results on Infrared Space Observatory (ISO) spectroscopic observations of Starburst and Ultraluminous Galaxies. Observations of a wide range of ionic, atomic, and molecular infrared lines enable us to explore in detail the physical conditions in the circumnuclear regions of these galaxies, and to determine, as a first step, parameters such as gas densities and temperatures of ionizing stars. With the help of theoretical modeling this multi-line spectroscopic database is used to further probe the central emission mechanism, discriminate between stellar and non-thermal processes and finally constrain the current models of galactic nuclei. |
| spellingShingle | Rigopoulou, D Lutz, D Genzel, R Egami, E Kunze, D Sturm, E ISO observations of starburst and ultraluminous galaxies |
| title | ISO observations of starburst and ultraluminous galaxies |
| title_full | ISO observations of starburst and ultraluminous galaxies |
| title_fullStr | ISO observations of starburst and ultraluminous galaxies |
| title_full_unstemmed | ISO observations of starburst and ultraluminous galaxies |
| title_short | ISO observations of starburst and ultraluminous galaxies |
| title_sort | iso observations of starburst and ultraluminous galaxies |
| work_keys_str_mv | AT rigopouloud isoobservationsofstarburstandultraluminousgalaxies AT lutzd isoobservationsofstarburstandultraluminousgalaxies AT genzelr isoobservationsofstarburstandultraluminousgalaxies AT egamie isoobservationsofstarburstandultraluminousgalaxies AT kunzed isoobservationsofstarburstandultraluminousgalaxies AT sturme isoobservationsofstarburstandultraluminousgalaxies |