Now showing items 1-2 of 2

    • Photon dominated regions in NGC 3603 [CI] and mid-J CO line emission 

      Röllig, M.; Kramer, C.; Rajbahak, C.; Minamidani, T.; Sun, K.; Simon, R.; Ossenkopf, V.; Cubick, M.; Hitschfeld, M.; Aravena, M.; Bensch, F.; Bertoldi, F.; Bronfman Aguiló, Leonardo; Fujishita, M.; Fukui, Y.; Graf, U. U.; Honingh, N.; Ito, S.; Jakob, H.; Jacobs, K.; Klein, U.; Koo, B.-C.; May Humeres, Jorge; Miller, M.; Miyamoto, Y.; Mizuno, N.; Onishi, T.; Park, Y.-S.; Pineda, J.; Rabanus, D.; Sasago, H.; Schieder, R.; Stutzki, J.; Yamamoto, H.; Yonekura, Y. (2011-01)
      Aims. We aim at deriving the excitation conditions of the interstellar gas as well as the local FUV intensities in the molecular cloud surrounding NGC 3603 to get a coherent picture of how the gas is energized by the central ...
    • Submillimeter line emission from LMC N159W: a dense, clumpy PDR in a low metallicity environment 

      Pineda, J. L.; Mizuno, Norikazu; Stutzki, J.; Cubick, M.; Aravena, Mauricio; Bensch, F.; Bertoldi, Frank; Bronfman Aguiló, Leonardo; Fujishita, K.; Graf, Urs U.; Hitschfeld, M.; Honingh, N.; Jakob, H.; Jacobs, K.; Kawamura, Akiko; Klein, U.; Kramer, C.; May Humeres, Jorge; Miller, M.; Mizuno, Yoji; Müller, P.; Onishi, T.; Ossenkopf, V.; Rabanus, David; Röllig, M.; Rubio López, Mónica; Sasago, H.; Schieder, R.; Simon, R.; Sun, K.; Volgenau, N.; Yamamoto, Hiroaki; Fukui, Yasuo (EDP SCIENCES S A, 2008-04)
      Context. Star formation at earlier cosmological times took place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation in such an environment. Aims. ...