Now showing items 1-3 of 3

    • Hitschfeld, M.; Aravena, M.; Kramer, C.; Bertoldi, F.; Stutzki, J.; Bensch, F.; Bronfman Aguiló, Leonardo; Cubick, M.; Fujishita, M.; Fukui, Y.; Graf, U.U; Honingh, N.; Ito, S.; Jakob, H.; Jacobs, K.; Klein, U.; Koo, B.-C.; May, J.; Miller, M.; Miyamoto, Y.; Mizuno, N.; Onishi, T.; Park, Y.-S.; Pineda, J. L.; Rabanus, D.; Röllig, M.; Sasago, H.; Schieder, R.; Simon, R.; Sun, K.; Volgenau, N.; Yamamoto, H.; Yonekura, Y. (EDP SCIENCES S A, 2008-02)
      Context. Studying molecular gas in the central regions of the star burst galaxies NGC4945 and Circinus enables us to characterize the physical conditions and compare them to previous local and high-z studies. Aims. We ...
    • 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 ...
    • 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. ...