Top Posters
Since Sunday
a
5
k
5
c
5
B
5
l
5
C
4
s
4
a
4
t
4
i
4
r
4
r
4
SlideshowReport

A Summary of Stellar Evolution

Description
A Summary of Stellar Evolution
(a) The evolution of isolated stars depends on their masses. The higher the mass, the shorter the lifetime. Stars less massive than about 8 solar
masses can eject enough mass to become white dwarfs. High-mass stars can produce Type II supernovae and become neutron stars or
black holes. The horizontal (time) axis is not to scale, but the relative lifetimes are accurate
Related Images
Add Comment
Explore
Post your homework questions and get free online help from our incredible volunteers
  1168 People Browsing
 114 Signed Up Today