| Lien | https://ui.adsabs.harvard.edu/abs/2006ASPC..356..266M/abstract |
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| Auteur | Rechercher : Matthews, Brenda C.1; Rechercher : Hogerheijde, Michiel; Rechercher : Bergin, Edwin |
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| Affiliation | - Conseil national de recherches du Canada. Institut Herzberg d'astrophysique du CNRC
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| Format | Texte, Article |
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| Conférence | Revealing the Molecular Universe: One Antenna Is Never Enough, September 9-10, 2005, Berkeley, California, USA |
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| Résumé | We present a BIMA molecular line study of the Class 0 source Barnard 1-c in the Perseus molecular cloud. As followup to the detection of an atypical polarization pattern in this young stellar object, we have obtained high resolution data in CO, C¹⁸O, ¹³CO, HCO⁺, and N₂H⁺ from BIMA, plus N₂H⁺ data from FCRAO. N₂H⁺ is destroyed in the core center and along the jet axis due to the high abundance of CO. The N₂H⁺ data demonstrate that this core is rotating with its rotation axis aligned with the observed molecular outflow. We have used high spectral resolution data of N₂H⁺ to measure the velocity and linewidths across the core. We find that B1-c exhibits similar morphology and kinematics to IRAM 04191+1522, another very young Class 0 source in Taurus. |
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| Date de publication | 2006 |
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| Dans | |
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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 | 13053852 |
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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 | 8ba0b44f-b42c-42cd-958a-8b7dcc1ece8d |
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| Enregistrement créé | 2009-11-25 |
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| Enregistrement modifié | 2021-03-04 |
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