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Why is the Star Formation Rate Proportional to Dense Gas Mass?

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Jiao, Sihan, Xu, Fengwei, Liu, Hauyu Baobab, Lin, Yuxin, Wu, Jingwen, Zhang, Zhi-Yu, Yan, Zhiqiang, Li, Di, Tsai, Chao-Wei, Zhang, Yongkun, Feng, Linjing, Wang, Ke, Zheng, Zheng, Meng, Fanyi, Ruan, Hao, Deng, Fangyuan, Su, Keyun
Format:	Preprint
Publié:	2025
Sujets:	Astrophysics of Galaxies
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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