Instituto de Astrofísica de AndalucíaMolecular gas
Scientific Results
Isolated galaxies
CO molecular gas content
CO molecular gas content We have CO(1-0) data for 273 AMIGA galaxies, most of them (n=186) from our own observations with the IRAM 30m and...
Chemistry in isolation
Chemistry in isolation Molecular abundances in the ISM have been shown to be imprinted by the different activity types in the nuclear region of galaxies....
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Compact groups
Strong far-infrared cooling lines, peculiar CO kinematics, and possible star-formation suppression in Hickson Compact Group 57
Strong far-infrared cooling lines, peculiar CO kinematics, and possible star-formation suppression in Hickson Compact Group 57 In this work, [C II] and [O I] observations...
Star formation suppression in compact group galaxies: a new path to quenching?
Star formation suppression in compact group galaxies: a new path to quenching? In the current work CO(1–0) maps of 12 warm H2-selected Hickson Compact Groups...
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