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Minamidani, TetsuhiroMizuno, NorikazuMizuno, YojiKawamura, AkikoOnishi, ToshikazuHasegawa, TetsuoTatematsu, Ken’ichiIkeda, MasafumiMoriguchi, YoshiakiYamaguchi, NobuyukiOtt, JürgenWong, TonyMuller, ErikPineda, Jorge L.Hughes, AnnieStaveley-Smith, ListerKlein, UlrichMizuno, AkiraNikolic, SilvanaBooth, Roy S.Heikkilä, ArtoNyman, Lars-AkeLerner, MikaelGaray Brignardello, GuidoKim, SungeunFujishita, MotosujiKawase, TokuichiRubio López, MónicaFukui, Yasuo[Submillimeter observations of giant molecular clouds in the Large Magellanic Cloud: Temperature and density as determined from J=3-2 and J=1-0 transitions of CO]

Garay Brignardello, GuidoJohansson, L. E. B.Nyman, L. A.Booth, Roy S.Israel, F. P.Kutner, M. L.Lequeux, J.Rubio López, Mónica[Results of the SEST Key Programme: CO in the Magellanic Clouds VIII. The giant molecular complex No. 37 of the LMC]

Israel, F. P.Graauw, Th. deJohansson, L.E.B.Booth, Roy S.Boulanger, FrancoisGaray Brignardello, GuidoKutner, M. L.Lequeux, J.Nyman, L. A.Rubio López, Mónica[Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds - IX - The giant LMC HII region complex N 11]

Israel, F. P.Johansson, L.E.B.Rubio López, MónicaGaray Brignardello, GuidoGraauw, Th. deBooth, Roy S.Boulanger, FrancoisKutner, M. L.Lequeux, J.Nyman, L.-A.[Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds X. CO emission from star formation regions in LMC and SMC]

Kutner, M. L.Rubio López, MónicaBooth, Roy S.Boulanger, FrancoisGraauw, Th. deGaray Brignardello, GuidoIsrael, F.P.Johansson, L.E.B.Lequeux, J.Nyman, L. A.[Results of the ESO-SEST key programme: CO in the Magellanic Clouds VI. The 30 Doradus Complex]

Rubio López, MónicaLequeux, J.Boulanger, FrancoisBooth, Roy S.Garay Brignardello, Guidode Graauw, Th.Israel, F. P.Johansson, L.E.B.Kutner, M.L.Nyman, L. A.[Results of the ESO-SEST Key Programme: CO in the Magellanic Clouds. V. Further CO observations of the Small Magellanic Cloud]

Sorai, K.Hasegawa, T.Booth, Roy S.Rubio López, MónicaMorino, J. I.Bronfman Aguiló, LeonardoHanda, T.Hatashi, M.Nyman, L. A.Oka, T.Sakamoto, S.Seta, M.Usuda, K. S.[The CO J = 21 / J = 10 Ratio in the Large Magellanic Cloud]

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