Koch, P. M.P. M.KochTang, Y. W.Y. W.TangHo, P. T. P.P. T. P.HoZhang, Q.Q.ZhangGirart, J. M.J. M.GirartChen, H. R. V.H. R. V.ChenLai, S. P.S. P.LaiLi, H. B.H. B.LiLi, Z. Y.Z. Y.LiLiu, H. B.H. B.LiuPadovani, MarcoMarcoPadovaniQiu, K.K.QiuRao, R.R.RaoYen, H. W.H. W.YenFrau, P.P.FrauChen, H. H.H. H.ChenChing, T. C.T. C.Ching2020-03-132020-03-132015978-2-7598-2022-11633-4760http://hdl.handle.net/20.500.12386/23217We highlight distinct and systematic observational features of magnetic field morphologies in polarized submm dust continuum. We illustrate this with specific examples and show statistical trends from a sample of 50 star-forming regions. <P />STAMPAenConference paper10.1051/eas/15750272-s2.0-84973909619000377836300026https://www.eas-journal.org/articles/eas/abs/2015/03/eas1575027/eas1575027.html2015EAS....75..159KFIS/05 - ASTRONOMIA E ASTROFISICA