Outflows and Bubbles in Taurus: Star-formation Feedback Sufficient to Maintain Turbulence
Huixian Li, Di Li, Lei Qian, Duo Xu, Paul F. Goldsmith, Alberto, Noriega-Crespo, Yuefang Wu, Yuzhe Song, Rendong Nan

TL;DR
This study identifies outflows and bubbles in Taurus, showing that stellar feedback from these phenomena is sufficient to sustain the cloud's turbulence despite not counteracting gravitational binding energy.
Contribution
First comprehensive mapping of outflows and bubbles in Taurus demonstrating their role in maintaining turbulence.
Findings
Outflows contribute about 1% of turbulent energy.
Bubbles contribute approximately 29% of turbulent energy.
Feedback energy rates are comparable to turbulence dissipation rates.
Abstract
We have identified outflows and bubbles in the Taurus molecular cloud based on the deg Five College Radio Astronomy Observatory CO(1-0) and CO(1-0) maps and the Spitzer young stellar object catalogs. In the main 44 deg area of Taurus we found 55 outflows, of which 31 were previously unknown. We also found 37 bubbles in the entire 100 deg area of Taurus, all of which had not been found before. The total kinetic energy of the identified outflows is estimated to be erg, which is \textbf{1\%} of the cloud turbulent energy. The total kinetic energy of the detected bubbles is estimated to be erg, which is 29\% of the turbulent energy of Taurus. The energy injection rate from outflows is , \textbf{0.4 - 2 times} the dissipation rate of the cloud turbulence.…
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