| Models
of Stellar Structure |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| • | Divide star into thin shells,calculate |
|||||||||||||
| how following vary from shell to |
||||||||||||||
| shell (i.e. as function of radius r) |
||||||||||||||
| – | P (Pressure) |
|||||||||||||
| – | T (Temperature) |
|||||||||||||
| – | (Density) |
|||||||||||||
| • | To
do this also need to find: |
|||||||||||||
| – | M
(Mass) contained within any r |
|||||||||||||
| – | L
(Luminosity) generated within any r |
|||||||||||||
| • | P example: |
|||||||||||||
