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Hydrodynamic model of a SN collapse and explosion
| Credit: |
Adam Burrows & John Hayes |
| Comments: |
The top set of
images links to a movie that follows the initial stages of the
core collapse. The bottom set links to a movie, which begins
near the end of the previous movie, and the scale has been
enlarged to follow the multi-dimensional explosion. |
| Publication: |
Burrows et al. 1995 |
|
 |
Hydrodynamic model of a SN collapse and explosion
| Credit: |
Adam Burrows & John Hayes |
| Comments: |
The colors indicate the electron fraction (Ye) |
| Publication: |
Burrows et al. 1995 |
|
 |
Hydrodynamic Model of a SNIa blast interacting with a main sequence star I
| Credit: |
Evonne Marietta |
| Comments: |
These results were featured on the cover of Nature in Feb. 2000. |
| Publication: |
Marietta et al. 2000 |
|
 |
Hydrodynamic Model of a SNIa blast interacting with a main sequence star II
| Credit: |
Evonne Marietta |
| Comments: |
This movie is different from the one above in that the distance
between the exploding star and the companion star is greater. |
| Publication: |
Marietta et al. 2000 |
|
 |
Hydrodynamic Model of a SNIa blast interacting with a main sequence star III
| Credit: |
Evonne Marietta |
| Comments: |
This movie focusses on the inner interaction regions during the
impact with a main sequence star. In addition, the velocity is represented by a vector field |
| Publication: |
Marietta et al. 2000 |
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sn50.gif
sn75.gif