Étude de différents progéniteurs de supernovæ

ρc∝T3
c
M2µ3

M&10M
(1)
(2)
15 40

M&10M
M∼2·1030 kg
(2)
r
(1.1.4)
r
P
∂P
∂r =−Gmρ r2,
m ρ r G = 6.673 ·10−8cm3g−1s−2
P=κργκ γ
(1.1) (A)
ρc
Tc
ρc∝T3
c
M2µ3,
M µ = (Ye+PiYi)−1YeYi
i
(1.1.2)
(1.2)
λ