Jiao, Sihan https://orcid.org/0000-0002-9151-1388
Xu, Fengwei https://orcid.org/0000-0001-5950-1932
Liu, Hauyu Baobab https://orcid.org/0000-0003-2300-2626
Lin, Yuxin https://orcid.org/0000-0001-9299-5479
Wu, Jingwen https://orcid.org/0000-0001-7808-3756
Zhang, Zhi-Yu https://orcid.org/0000-0002-7299-2876
Yan, Zhiqiang https://orcid.org/0000-0001-7395-1198
Li, Di https://orcid.org/0000-0003-3010-7661
Tsai, Chao-Wei https://orcid.org/0000-0002-9390-9672
Zhang, Yongkun https://orcid.org/0000-0002-8744-3546
Feng, Linjing https://orcid.org/0009-0003-4821-5502
Wang, Ke https://orcid.org/0000-0002-7237-3856
Zheng, Zheng https://orcid.org/0009-0005-9546-4573
Meng, Fanyi https://orcid.org/0000-0002-5927-2049
Ruan, Hao
Deng, Fangyuan https://orcid.org/0009-0003-9223-2297
Su, Keyun https://orcid.org/0009-0003-2243-7983
Funding for this research was provided by:
National Science and Technology Council (111-2112-M-110-022-MY3)
National Science and Technology Council (113-2112-M-110-022-MY3)
MOST ∣ NSFC ∣ Joint Fund of Astronomy (12588202)
MOST ∣ NSFC ∣ Joint Fund of Astronomy (12041302)
Article Title: Why is the Star Formation Rate Proportional to Dense Gas Mass?
Journal Title: The Astrophysical Journal
Article Type: paper
Copyright Information: © 2025. The Author(s). Published by the American Astronomical Society.
Publication dates
Date Received: 2024-08-16
Date Accepted: 2025-04-23
Online publication date: 2025-06-30