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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 B2.

Scatter plots showing the relationships between distance and the physical quantities shown in Figure 5. The Pearson correlation coefficients and corresponding p-values are labeled in the top left corner of each panel. An additional physical quantity, the core size (FWHM﹩=\sqrt{{\theta }_{{\rm{mag}}}{\theta }_{{\rm{\min }}}}﹩, where θ_mag and ﹩{\theta }_{{\rm{\min }}}﹩ are listed in Table E1), is displayed in the last panel.

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