| DOI | Trouver le DOI : https://doi.org/10.1017/S1743921304002297 |
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| Auteur | Rechercher : Shastri, Prajval; Rechercher : Murthy, Jayant; Rechercher : Hutchings, John1; Rechercher : Wills, Beverley J. |
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| Affiliation | - Conseil national de recherches Canada. Institut Herzberg d'astrophysique du CNRC
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| Format | Texte, Article |
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| Résumé | We present our recent results from the observation of the O VI λ λ1032,1038 emission doublet in Seyfert galaxies of type 2 with the FUV spectrograph on the FUSE satellite. These observations are part of our investigation to contrast the properties of the OVI emission line and the absorbing outflows in a sample of rigorously matched Seyfert 1s and 2s, in the framework of the Unified Scheme. The OVI emission line is an excellent diagnostic of the outflowing hot gas at temperatures of ∼10⁶K. In the Unified Scheme, Seyferts of type 2 are those whose central regions are obscured by the ubiquitous dusty torus. We interpret our results in this framework.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html |
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| Date de publication | 2004-11-24 |
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| Série | |
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| Langue | anglais |
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| Publications évaluées par des pairs | Oui |
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| Numéro NPARC | 13053318 |
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| Exporter la notice | Exporter en format RIS |
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| Signaler une correction | Signaler une correction (s'ouvre dans un nouvel onglet) |
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| Identificateur de l’enregistrement | c522aab0-3b0e-4ada-af40-3911288f39fb |
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| Enregistrement créé | 2009-11-25 |
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| Enregistrement modifié | 2020-04-17 |
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