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    • Minier, V.; Tremblin, P.; Hill, T.; Motte, F.; André, Ph.; Lo, N.; Schneider, N.; Audit, E.; White, G. J.; Hennemann, M.; Cunningham, M.; Deharveng, L.; Di Francesco, J.; Elia, D.; Giannini, T.; Luong, Q. Nguyen; Pezzuto, S.; Rygl, K. L.; Spinoglio, L.; Ward Thompson, D.; Zavagno, A. (EDP Sciences, 2013)
      Context. Ionising stars reshape their original molecular cloud and impact star formation, leading to spectacular morphologies such as bipolar nebulae around Hii regions. Molecular clouds are structured in filaments where ...