ALMAGAL

S'anchez-Monge, A.; L. Brogan, C.; R. Hunter, T.; Ahmadi, A.; Avison, A.; Beltr'an, M.T.; Beuther, H.; Coletta, Alessandro; A. Fuller, G.; Johnston, K.; Jones, B.; Liu, Sheng‐Yuan; Mininni, C.; Molinari, S.; Schilke, P.; Schisano, E.; Su, Yang; Traficante, A.; Zhang, Qizhou; Battersby, C.; Benedettini, M.; Elia, D.; T. P. Ho, Paul; Klaassen, Pamela; S. Klessen, Ralf; Law, Chi-Yan; Lis, D.C.; Liu, Tie; T. Maud, L.; Möller, T.; Moscadelli, L.; Pezzuto, S.; L. J. Rygl, K.; Sanhueza, P.; D. Soler, J.; Stroud, G.; Tang, Yongan; S. van der Tak, Floris; L. Walker, Denise; Wallace, J.; Walch, S.; R. A. Wells, M.; Wyrowski, F.; Zhang, Tianwei; Allande, J.; Bronfman, L.; Dann, E.; De Angelis, F.; Fontani, F.; Henning, Th.; Kim, W.-J.; Kuiper, R.; Merello, Manuel; Nakamura, F.; Nucara, A.; J. Rigby, A.

doi:10.1051/0004-6361/202452703

Public

ALMAGAL

Published in Astronomy and Astrophysics • Mar 14, 2025

Authors:

A. S'anchez-Monge

C. L. Brogan

T. R. Hunter

Abstract

Context. Stars form preferentially in clusters embedded inside massive molecular clouds, many of which contain high-mass stars. Thus, a comprehensive understanding of star formation requires a robust and statistically well-constrained characterization of the formation and early evolution of these hi...

Subject

Physics

Astrophysics

Galaxy

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