Dynamical accretion flows: ALMAGAL: flows along filamentary structures in high-mass star-forming clusters
- Author(s):
- Wells, M.R.A.; Beuther, H.; Molinari, S.; Schilke, P.; Battersby, C.; Ho, P.; Sánchez-Monge, Á.; Jones, B.; Scheuck, M.B.; Syed, J.; Gieser, C.; Kuiper, R.; Elia, D.; Coletta, A.; Traficante, A.; Wallace, J.; Rigby, A.J.; Klessen, R.S.; Zhang, Q.; Walch, S.; Beltrán, M.T.; Tang, Y.; Fuller, G.A.; Lis, D.C.; Möller, T.; van der Tak, F.; Klaassen, P.D.; Clarke, S.D.; Moscadelli, L.; Mininni, C.; Zinnecker, H.; Maruccia, Y.; Pezzuto, S.; Benedettini, M.; Soler, J.D.; Brogan, C.L.; Avison, A.; Sanhueza, P.; Schisano, E.; Liu, T.; Fontani, F.; Rygl, K.L.J.; Wyrowski, F.; Bally, J.; Walker, D.L.; Ahmadi, A. (0000-0003-4037-5248); Koch, P.; Merello, M.; Law, C.Y.; Testi, L.
- Published
- 2024
- Publication type
- Article / Letter to editor
- Date issued
- 2024
- Language
- English
- Is part of
- Astronomy & Astrophysics (2024), A185
- hdl
- 1887/4179081
- doi
- 10.1051/0004-6361/202449794
- URL
- https://ui.adsabs.harvard.edu/abs/2024A&A...690A.185W
