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  • Greve, T. R; Leonidaki, I; Xilouris, E.M; Weiss, A; Zhang, Z.-Y; van der Werf, P; Aalto, S; Armus, L; Diaz-Santos, T; Evans, A.S; Fischer, J; Gao, Y; Gonzalez-Alfonso, E; Harris, A; Henkel, C; Mekjerink, R; Naylor, D.A; Smith, H.A; Spaans, M; Stacey, G.J; Veilleux, S; Walter, F (American Astronomical Society, 2014)
    We present FIR[50 􀀀 300 m]􀀀CO luminosity relations (i.e., log LFIR = log L0 CO + ) for the full CO rotational ladder from J = 1 􀀀 0 up to J = 13 􀀀 12 for a sample of 62 local (z 0:1) (Ultra) Luminous Infrared ...
  • Kohler, M.; Habart, E; Arab, H; Bernard-Salas, J; Ayasso, H; Abergel, A; Zavagno, A; Polehampton, E; van der Wiel, M.H.D; Naylor, D.A; Makiwa, G; Dassas, K; Joblin, C; Pilleri, P; Berne, O; Fuente, A; Gerin, M; Goicoechea, J.R; Teyssier, D (Springer-Verlag, 2014)
    Context. The determination of the physical conditions in molecular clouds is a key step towards our understanding of their formation and evolution of associated star formation. We investigate the density, temperature, and ...