Browsing by Author "Hennemann, M."

Now showing items 1-2 of 2

    • Ionisation impact of high-mass stars on interstellar filaments A Herschel study of the RCW36 bipolar nebula ... 
      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 ...
    • Low-velocity shocks traced by extended sio emission along the w43 ridges: witnessing the formation of young ... 
      Nguyen-Luong, Q.; Motte, F.; Carlhoff, P.; Louvet, F.; Lesaffre, P.; Schilke, P.; Hill, T.; Hennemann, M.; Gusdorf, A.; Didelon, P.; Schneider, N.; Bontemps, S.; Duarte Cabral, A.; Menten, K. M.; Martin, P. G.; Wyrowski, F.; Bendo, G.; Roussel, H.; Bernard, J. P.; Bronfman Aguiló, Leonardo; Henning, Thomas; Kramer, C.; Heitsch, F. (The American Astronomical Society, 2013-10-01)
      The formation of high-mass stars is tightly linked to that of their parental clouds. Here, we focus on the high-density parts of W43, a molecular cloud undergoing an efficient event of star formation. Using a column density ...