Ident. | Title | Freq. (GHz) | Authors |
19.95 | Do the PIGs in M42 contain molecular material ? | 113, 226, 110, 219, 146 | Rodriguez, Martin-Pintado, Fuente |
63.95 | A new class of molecular clouds in the galactic center region | 86, 91, 130, 214, 220 | Martin-pintado, Fuente, de Vicente |
75.95 | Probing the H /H transition layer in PDRS | 115, 162, 208, 235, 89 | Fuente, Martin-Pintado |
35.95 | The hot molecular ring around the Sgr B2 star forming cores | 91, 147, 220, 102, 222 | De Vicente, Martin-Pintado |
20.95 | Does dense material confine HII regions ? | 108, 113, 145, 109, 218 | Martin-pintado, Gaume, Rodriguez, de Pree, Fey |
14.95 | CO observations of H O megamaser active galaxies | 113, 226, 229 | Planesas, Colina, Raluy |
44.95 | Observational tests of chemical bistability in dense interstellar clouds | 115, 230 | Gerin, Falgarone, Roueff, Pineau des Forets |
43.95 | Formation of CO along a dissipation region within a high galactic latitude HI cloud | 115, 230 | Boulanger, Falgarone, Zagury |
74.95 | L483 : The birth of a cometary nebula | 96, 110, 130, 140, 230 | Tafalla, Mardones, Myers, Bachiller, Fuller |
23.95 | The main molecular Bar of NGC 4321 | 114, 229 | Sempere, Garcia-Burillo, Combes |
55.95 | Chemical evolution in the outer galaxy | 109, 115, 219, 224 | Henkel, wouterloot, Mauersberger, Brand, Chin |
85.95 | H O emission from a circumnuclear disk | 96, 232 | Henkel |