Abstract Mass loss is a key process in the evolution of massive stars, and must be understood quantitatively if it is to be successfully included in broader astrophysical applications such as galactic and cosmic evolution and ionization.
[...]
|
||||||
|
|
||||||
|
|
||||||
|
||||||
|
Abstract Mass loss is a key process in the evolution of massive stars, and must be understood quantitatively if it is to be successfully included in broader astrophysical applications such as galactic and cosmic evolution and ionization. |
||||||
|
|
||||||