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| Deletions are marked like this. | Additions are marked like this. |
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| || Abs || Watts || 10 pc || 100 pc || || Mag || || W/m² || W/m² || || -19 || 1.2e36 || 100 || 1.00 || || -18 || 4.8e35 || 40 || 0.40 || || -17 || 1.9e35 || 16 || 0.16 || || -16 || 7.6e34 || 6.3 || 63m || || -15 || 3.0e34 || 2.5 || 25m || || -14 || 1.2e34 || 1.0 || 10m || || -13 || 4.8e33 || 0.4 || 4m || ||<-3> gamma and X rays || || distance || sn1a || snII || || || 2e34W ||1e32W || || pc || W/m² || W/m² || || 10 || 16.7m || 84μ || || 30 || 1.86m || 9.3μ || || 100 || 167μ || 840n || || 300 || 18.6μ || 93n || || 1000 || 1.67μ || 8.4n || |
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| {{attachment:Comparative_supernova_type_light_curves.png}} | [[attachment:Comparative_supernova_type_light_curves.png|{{attachment:Comparative_supernova_type_light_curves.png| |width=800}}]] -------- . Stellar Interiors by Hansen+ QB808 H36 1994 . Table 6.3 p 247 . C + C → Ne + α 44% . . . C + C → Na + p 56% . O + O → Si + α 21% . . . O + O → P + p 61% . . . O + O → Si + n 18% . Thielemann and Arnett 1985 2x downloaded . Truran 1966 (paywall) . Bodansky Clayton Fowler 1968 2x downloaded . Section 6.8 p251 Neutrino emission mechanisms . When temperatures are high enough - kT ~ 2 m,,e,,c² photons creates electron positron pairs . Ordered this book! |
Supernova effects on Server Sky and Stady Shell
The Sun's absolute bolometric (all band) magnitude is +4.74, 3.828 e26 W, so an absolute magnitude of zero is 3.013e28 W.
Abs |
Watts |
10 pc |
100 pc |
Mag |
|
W/m² |
W/m² |
-19 |
1.2e36 |
100 |
1.00 |
-18 |
4.8e35 |
40 |
0.40 |
-17 |
1.9e35 |
16 |
0.16 |
-16 |
7.6e34 |
6.3 |
63m |
-15 |
3.0e34 |
2.5 |
25m |
-14 |
1.2e34 |
1.0 |
10m |
-13 |
4.8e33 |
0.4 |
4m |
||<-3> gamma and X rays ||
distance |
sn1a |
snII |
|
2e34W |
1e32W |
pc |
W/m² |
W/m² |
10 |
16.7m |
84μ |
30 |
1.86m |
9.3μ |
100 |
167μ |
840n |
300 |
18.6μ |
93n |
1000 |
1.67μ |
8.4n |
Type Ia |
2e44 J |
Supernovae Light Curves:
- Stellar Interiors by Hansen+ QB808 H36 1994
- Table 6.3 p 247
- C + C → Ne + α 44% . . . C + C → Na + p 56%
- O + O → Si + α 21% . . . O + O → P + p 61% . . . O + O → Si + n 18%
- Thielemann and Arnett 1985 2x downloaded
- Truran 1966 (paywall)
- Bodansky Clayton Fowler 1968 2x downloaded
- Section 6.8 p251 Neutrino emission mechanisms
When temperatures are high enough - kT ~ 2 mec² photons creates electron positron pairs
- Ordered this book!