A compact starburst ring traced by clumpy OH megamaser emission
We model the OH megamaser emission from the luminous infrared galaxy IIIZw35 as arising from a narrow rotating starburst ring of radius 22 pc enclosing a mass of 7 . We show how both the compact and apparently diffuse maser emission from this ring can arise from a single phase of unsaturated maser c...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2005-11, Vol.443 (2), p.383-396 |
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Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | We model the OH megamaser emission from the luminous infrared galaxy IIIZw35 as arising from a narrow rotating starburst ring of radius 22 pc enclosing a mass of 7 . We show how both the compact and apparently diffuse maser emission from this ring can arise from a single phase of unsaturated maser clouds amplifying background radio continuum. The masing clouds are estimated to have a diameter of |
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ISSN: | 0004-6361 1432-0746 |
DOI: | 10.1051/0004-6361:20052971 |