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The ALMA-QUARKS Survey: Investigating Thermal Feedback of Massive Protostars in Hot Molecular Cores

  • Authors: Dezhao Meng, Tie Liu, Jarken Esimbek, Yisheng Qiu, Jixing Ge, Neal J. Evans, Aina Palau, Guido Garay, Paul F. Goldsmith, Fengwei Xu, Sami Dib, Jeong-Eun Lee, Amelia M. Stutz, Xindi Tang, Xiaofeng Mai, Yan-Kun Zhang, Wenyu Jiao, Jia-Hang Zou, Leonardo Bronfman, Swagat R. Das, Prasanta Gorai, Jian-Wen Zhou, Pablo García, L. Viktor Tóth, Sheng-Yuan Liu, Patricio Sanhueza, Chang Won Lee, Kee-Tae Kim, Jianjun Zhou, Gang Wu, Dalei Li, Yuxin He, Dongting Yang, James O. Chibueze, Xunchuan Liu, Lei Zhu

Dezhao Meng et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure C1.

Model results (color-coded lines with filled circles or squares) with fitted abundance profiles (solid gray lines with different parameters). The color-coded lines with points and squares are for models Tmedian and Tfunc respectively. The black lines show temperature profiles used in our two models: Tmedian and Tfunc (right axis). Temperature of 150 K are marked for the two temperature profiles with red vertical lines. At the bottom, small vertical lines indicate radii with a modeled abundance of 0.85Xpeak, serving as a rough estimation of break radii from the models. Note: T(r) = Tfunc.

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