Distribution of star formation in galactic bars as seen in the S4G survey
The torques exerted by stellar bars are expected to provoke the flow of cold gas within the disk, driving the secular evolution of the inner parts of the galaxy, as established in simulation models since the last century. To date, it remains a matter of debate why the distribution of ionized gas along bars and in the circumnuclear regions varies
Díaz-García, S. et al.
Advertised on:
1
2021