Abstract
2D calculations of the evolution of the remnants generated by the strong mechanical energy produced by a central starburst in dwarf galaxies are presented. We show how the extended H I halos inhibit a galactic wind and thus the exit of metals from these galaxies.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
