From haloes to galaxies -- II. The fundamental relations in star formation and quenching
Jing Dou, Yingjie Peng, Alvio Renzini, Luis C. Ho, Filippo Mannucci,, Emanuele Daddi, Yu Gao, Roberto Maiolino, Chengpeng Zhang, Qiusheng Gu, Di, Li, Simon J. Lilly, Feng Yuan

TL;DR
This paper investigates the fundamental relations among galaxy properties like stellar mass, star formation rate, and molecular gas, proposing a new core relation that underpins galaxy evolution and explains other observed scaling laws.
Contribution
It introduces the sSFR-$$-SFE relation as the Fundamental Formation Relation (FFR), unifying various galaxy scaling laws and providing insights into star formation and quenching processes.
Findings
The sSFR-$$-SFE relation has minimal scatter, indicating a fundamental physical connection.
Other key relations can be derived from the FFR, including the Kennicutt-Schmidt law.
Systematic dependencies cause larger scatter in some relations, linked to star formation and quenching.
Abstract
Star formation and quenching are two of the most important processes in galaxy formation and evolution. We explore in the local Universe the interrelationships among key integrated galaxy properties, including stellar mass , star formation rate (SFR), specific SFR (sSFR), molecular gas mass , star formation efficiency (SFE) of the molecular gas and molecular gas to stellar mass ratio . We aim to identify the most fundamental scaling relations among these key galaxy properties and their interrelationships. We show the integrated -SFR, SFR- and - relation can be simply transformed from the -sSFR, SFE- and SFE-sSFR relation, respectively. The transformation, in principle, can increase or decrease the scatter of each relation. Interestingly, we find the latter three relations all have significantly smaller scatter than the…
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