Elia, D, Coletta, A, Molinari, S, Schisano, E, Benedettini, M, Sánchez-Monge, Á, Traficante, A, Mininni, C, Nucara, A, Pezzuto, S, Schilke, P, Soler, JD, Avison, A, Beltrán, MT, Beuther, H, Clarke, S, Fuller, GA, Klessen, RS, Kuiper, R, Lebreuilly, U, Lis, DC, Möller, T, Moscadelli, L, Rigby, AJ, Sanhueza, P, van der Tak, F, Zhang, Q, Rygl, KLJ, Merello, M, Battersby, C, Ho, PTP, Klaassen, PD, Koch, PM, Allande, J, Bronfman, L, Fontani, F, Hennebelle, P, Jones, BM, Liu, T, Stroud, G, Wells, MRA, Ahmadi, A, Brogan, CL, De Angelis, F, Hunter, TR, Johnston, KG, Law, CY, Liu, SJ, Liu, SY, Maruccia, Y, Pelkonen, VM, Su, YN, Tang, Y, Testi, L, Walch, S
, Zhang, T & Zinnecker, H 2026, '
ALMAGAL. V. Relations between the core populations and the parent clump physical properties',
Astronomy and Astrophysics, vol. 705, pp. A100. <
https://doi.org/10.1051/0004-6361/202554764>