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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 8.

Left panel: comparison of different mass scales as a function of the embedded protostellar luminosity, L. The crosses show the thermal Jeans mass, MJeans, versus L. The blue solid line shows the ZAMS stellar mass, M, as a function of L (D. Szécsi et al. 2022; P. Hennebelle & M. Y. Grudić 2024). The red dashed line shows the relation between the envelope mass, Menv, and L (Figure 7(c)). Right panel: the scatter between the envelope mass and thermal Jeans mass. The dashed gray line presents y = x. The purple crosses indicate dust-ff hot cores, and the blue ones represent the rest of the hot cores.

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