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Outflows and Bubbles in Taurus: Star-formation Feedback Sufficient to Maintain Turbulence
We have identified outflows and bubbles in the Taurus molecular cloud based on the \(\sim 100\) deg\(^2\) Five College Radio Astronomy Observatory \(^{12}\)CO(1-0) and \(^{13}\)CO(1-0) maps and the Spitzer young stellar object catalogs. In the main 44 deg\(^2\) area of Taurus we found 55 outflows, o...
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Published in: | arXiv.org 2015-08 |
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Main Authors: | , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
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Summary: | We have identified outflows and bubbles in the Taurus molecular cloud based on the \(\sim 100\) deg\(^2\) Five College Radio Astronomy Observatory \(^{12}\)CO(1-0) and \(^{13}\)CO(1-0) maps and the Spitzer young stellar object catalogs. In the main 44 deg\(^2\) area of Taurus we found 55 outflows, of which 31 were previously unknown. We also found 37 bubbles in the entire 100 deg\(^2\) area of Taurus, all of which had not been found before. The total kinetic energy of the identified outflows is estimated to be \(\bf \sim 3.9 \times 10^{45}\) erg, which is \textbf{1\%} of the cloud turbulent energy. The total kinetic energy of the detected bubbles is estimated to be \(\sim 9.2 \times 10^{46}\) erg, which is 29\% of the turbulent energy of Taurus. The energy injection rate from outflows is \(\bf \sim 1.3 \times 10^{33}~\rm erg\ s^{-1}\), \textbf{0.4 - 2 times} the dissipation rate of the cloud turbulence. The energy injection rate from bubbles is \(\sim 6.4 \times 10^{33}\) erg s\(^{-1}\), \textbf{2 - 10 times} the turbulent dissipation rate of the cloud. The gravitational binding energy of the cloud is \(\bf \sim 1.5 \times 10^{48}\) {\bf erg}, \textbf{385} and 16 times the energy of outflows and bubbles, respectively. We conclude that neither outflows nor bubbles can \textbf{provide enough energy to balance the overall gravitational binding energy and the turbulent energy of Taurus. However,} in the current epoch, stellar feedback is sufficient to maintain the observed turbulence in Taurus. |
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ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.1507.06512 |