The C-flash and the ignition conditions of type Ia supernovae
Thanks to a stellar evolution code able to compute through the C-flash we link the binary population synthesis of single degenerate progenitors of type Ia supernovae (SNe Ia) to their physical condition at the time of ignition. We show that there is a large range of possible ignition densities and...
| Main Authors: | , , , , |
|---|---|
| Format: | Journal article |
| Published: |
2006
|