Why is the Star Formation Rate Proportional to Dense Gas Mass?
Sihan Jiao, Fengwei Xu, Hauyu Baobab Liu, Yuxin Lin, Jingwen Wu, Zhi-Yu Zhang, Zhiqiang Yan, Di Li, Chao-Wei Tsai, Yongkun Zhang, Linjing Feng, Ke Wang, Zheng Zheng, Fanyi Meng, Hao Ruan, Fangyuan Deng, and Keyun Su

TL;DR
This paper uncovers a correlation between the maximum core mass and bound gas mass in molecular clouds, suggesting the Gao-Solomon relation arises from interconnected star formation processes and core-to-star efficiency, offering an analytic understanding.
Contribution
It demonstrates a significant correlation between core and gas masses and links this to the Gao-Solomon relation through theoretical relations, providing a new perspective on star formation laws.
Findings
Discovered a correlation between maximum core mass and bound gas mass.
Proposed the Gao-Solomon relation results from interconnected star formation relations.
Suggested a theoretical framework linking core properties to star formation rate.
Abstract
One of the most profound empirical laws of star formation is the Gao-Solomon relation, a linear correlation between the star formation rate (SFR) and the dense molecular gas mass. It is puzzling how the complicated physics in star-formation results in this surprisingly simple proportionality. Using archival Herschel and Atacama Large Millimeter/submillimeter Array Observations, we derived the masses of the most massive cores () and masses of the gravitationally bound gas () in the parent molecular clouds for a sample of low-mass and high-mass star-forming regions. We discovered a significant correlation . Our discovered - correlation can be approximately converted to the Gao-Solomon relation if…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Fullerene Chemistry and Applications · Dust and Plasma Wave Phenomena
