18
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)
–r (Density)
•To
do this also need to find:
–M
(Mass) contained
within any r
–L
(Luminosity) generated within
any r
•P example:
From our text: Horizons, by Sees