Molecular gas and star formation within 12 strong galactic bars observed with IRAM-30 m
Context. While some galactic bars show recent massive star formation (SF) along them, some others do not. Whether bars with low level of SF are a consequence of low star formation efficiency, low gas inflow rate, or dynamical effects remains a matter of debate. Aims: In order to study the physical conditions that enable or prevent SF, we perform a
Díaz-García, S. et al.
Fecha de publicación:
10
2021