Link | https://ui.adsabs.harvard.edu/abs/2006ASPC..356..266M/abstract |
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Author | Search for: Matthews, Brenda C.1; Search for: Hogerheijde, Michiel; Search for: Bergin, Edwin |
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Affiliation | - National Research Council of Canada. NRC Herzberg Institute of Astrophysics
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Format | Text, Article |
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Conference | Revealing the Molecular Universe: One Antenna Is Never Enough, September 9-10, 2005, Berkeley, California, USA |
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Abstract | 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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Publication date | 2006 |
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In | |
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Series | |
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Language | English |
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Peer reviewed | Yes |
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NPARC number | 13053852 |
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Export citation | Export as RIS |
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Report a correction | Report a correction (opens in a new tab) |
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Record identifier | 8ba0b44f-b42c-42cd-958a-8b7dcc1ece8d |
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Record created | 2009-11-25 |
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Record modified | 2021-03-04 |
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