The Chemical Evolution of Very Metal-Poor Damped LYα Systems
In earlier work we showed that a dark matter halo with a virial mass of 107 M⊙ can survive feedback from its own massive stars and form stars for ≳100 Myr. We also found that our modeled systems were consistent with observations of ultrafaint dwarfs (
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|Access Rights:||Open Access|
|01_Webster_The_Chemical_Evolution_of_Very_2015.pdf||2.57 MB||Adobe PDF|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.