Stellar evolution of low and intermediate-mass-stars. II. Post-AGB evolution. J/A+A/299/755 J/A+A/299/755 Stellar evolution. II. Post-AGB Stellar evolution of low and intermediate-mass-stars. II. Post-AGB evolution. T Bloecker Astron. Astrophys. 299 755 1995 1995A&A...299..755B stars: AGB and post-AGB stars: evolution stars: mass-loss white dwarfs We present a set of evolutionary tracks for central stars of planetary nebulae in the range from 0.53 to 0.94M_{sun}_. These models are based on extensive stellar evolution calculations for initial masses between 1 and 7M_{sun}_ which have been carried out all the way from the main sequence through the AGB towards the stage of white dwarfs.
Data for hydrogen burning models Data for hydrogen burning models Data for helium burning models Minitial Initial mass solMass Mfinal Final mass solMass Age Post-AGB age yr log(Teff) Effective temperature K log(L) Luminosity solLum Patricia Bauer CDS 1995Feb21Thomas Bloecker <tbloecker@aip.de> J_A+A_299_755.xml