Initial
Mass Final Mass Composition
______________________________________________
0.08
- 0.25 0.05 - 0.2 He
0.25
- 8 0.5 - 1.4 C,O
8
- 10 0.5 - 1.4 O,Ne,Mg
______________________________________________
Radii
– typically 1000-5000 km (smaller than Earth!)
Luminosities
– 10-2 to 10-5 solar luminosities
Densities
– typically 105 to 107 gm/cc
Temperatures
– anywhere from 100,000 to 2500 K.
The small
radii and luminosities mean that we can only see them if close-by,
or by their effects in binary systems.