The dominance of turbulence over magnetism in the formation of massive star cluster seeds

Fuente: arXiv

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Bibliographic Details
Main Authors:	Liu, Junhao, Sanhueza, Patricio, Saha, Piyali, Morii, Kaho, Girart, Josep Miquel, Zhang, Qizhou, Nakamura, Fumitaka, Cortes, Paulo C., Valdivia, Valeska, Commercon, Benoit, Koch, Patrick M., Pattle, Kate, Lu, Xing, Karoly, Janik, Fernandez-Lopez, Manuel, Stephens, Ian W., Chen, Huei-Ru Vivien, Law, Chi-Yan, Qiu, Keping, Li, Shanghuo, Beuther, Henrik, Chung, Eun Jung, Wang, Jia-Wei, Olguin, Fernando A., Cheng, Yu, Hwang, Jihye, Panigrahy, Sandhyarani, Eswaraiah, Chakali, Beltran, Maria T., Luo, Qiuyi, Choudhury, Spandan, Kang, Ji-hyun, Jiao, Wenyu, Zapata, Luis A., Lyo, A. -Ran
Format:	Preprint
Published:	2026
Subjects:	Astrophysics of Galaxies Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2603.17254