Ultrafaint dwarfs - Star formation and chemical evolution in the smallest galaxies
In earlier work, we showed that a dark matter halo with a virial mass of 107 M ⊙ can retain a major part of its baryons in the face of the pre-ionization phase and supernova (SN) explosion from a 25 M ⊙ star. Here, we expand on the results of that wor
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Webster_Ultrafaint_dwarfs_-_Star_2014.pdf||1.94 MB||Adobe PDF|
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