Molecular gas in low-metallicity starburst galaxies:. Scaling relations and the CO-to-H2 conversion factor
Context. Tracing the molecular gas-phase in low-mass star-forming galaxies becomes extremely challenging due to significant UV photo-dissociation of CO molecules in their low-dust, low-metallicity ISM environments. Aims: We aim to study the molecular content and the star-formation efficiency of a representative sample of 21 blue compact dwarf
Amorín, R. et al.
Fecha de publicación:
4
2016