| Télécharger | - Voir la version finale : The JCMT Gould Belt Survey : SCUBA-2 observations of radiative feedback in NGC 1333 (PDF, 819 Ko)
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| DOI | Trouver le DOI : https://doi.org/10.1093/mnrasl/sls015 |
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| Auteur | Rechercher : Hatchell, J.; Rechercher : Wilson, T.; Rechercher : Drabek, E.; Rechercher : Curtis, E.; Rechercher : Richer, J.; Rechercher : Nutter, D.; Rechercher : Di Francesco, J.1; Rechercher : Ward-Thompson, D. |
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| Affiliation du nom | - Conseil national de recherches du Canada. Herzberg en astronomie et en astrophysique
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| Format | Texte, Article |
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| Sujet | stars: formation; dust; extinction; submillimetre: ISM; stars: protostars |
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| Résumé | We present observations of NGC 1333 from SCUBA-2 on the James Clerk Maxwell Telescope (JCMT), observed as a JCMT Gould Belt Survey pilot project during the shared risk campaign when the first of four arrays was installed at each of 450 and 850 μm. Temperature maps are derived from 450 and 850 μm ratios under the assumption of constant dust opacity spectral index β = 1.8. Temperatures indicate that the dust in the northern (IRAS 6/8) region of NGC 1333 is hot, 20–40 K, due to heating by the B star SVS3, other young stars in the IR/optically visible cluster and embedded protostars. Other luminous protostars are also identified by temperature rises at the 17 arcsec resolution of the ratio maps (0.02 pc assuming a distance of 250 pc for Perseus). The extensive heating raises the possibility that the radiative feedback may lead to increased masses for the next generation of stars. |
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| Date de publication | 2013-02-11 |
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| Maison d’édition | The authors on behalf of the JCMT GBS Consortium (Oxford) |
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| Dans | |
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| Langue | anglais |
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| Publications évaluées par des pairs | Oui |
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| Numéro NPARC | 23001799 |
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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 | 20ef263d-6b06-4e58-bff9-df04444e7a41 |
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| Enregistrement créé | 2017-04-07 |
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| Enregistrement modifié | 2020-05-30 |
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