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The Evolution of Protostellar Outflow Cavities, Kinematics, and Angular Distribution of Momentum and Energy in Orion A: Evidence for Dynamical Cores

  • Authors: Cheng-Han Hsieh, 承翰 謝, Héctor G. Arce, Zhi-Yun Li, Michael Dunham, Stella Offner, Ian W. Stephens, Amelia Stutz, Tom Megeath, Shuo Kong, Adele Plunkett, John J. Tobin, Yichen Zhang, Diego Mardones, Jaime E. Pineda, Thomas Stanke, John Carpenter

Cheng-Han Hsieh et al 2023 The Astrophysical Journal 947 .

  • Provider: AAS Journals

Caption: Figure 9.

Profiles of the average molecular outflow mass, momentum, and energy rates per outflow lobe for different protostellar evolutionary classes (Class 0, Class I, and flat spectrum). For the Class 0 sources, we show the average rates with and without inclusion of the high-velocity jet component. All results shown are inclination corrected. In creating these plots, the Class 0 source HOPS 408 was not included because its outflow is barely resolved, and the flat-spectrum sources HOPS 166 and HOPS 194 were not included because they have significantly higher bolometric luminosity (>10 L ) and significantly higher core masses compared to other sources in this study. The dispersion of outflow rate values for each evolutionary class is approximately a factor of 2.

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