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The helium burning evolution of low mass stars

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Figure

TABLE  OF  CONTENTS
Figure  1  shows  the  track  of  the  star  in  the  theoretical  H-R  diagram  from  the  HB  to  the  region  occupied  by  planetary  nebula  nuclei
FIG.  1.  - The  evolutionary  track  in  the  H-R  diagram  of  a  0.6
FIG.  2.  - The  variation  of  the  luminosity  of  the  helium  shell  i  wi th  time  on  the  upper  asymptotic  branch
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