Stellar Evolution Figures (Caroll & Ostlie, Laughlin et al., etc.)

• Gravitational collapse

  • Grav. collapse, 1 Msun : HR track + times [CO-1e Fig 12.7] (Appenzeller & Tscharnuter 1975)
  • Grav. collapse, 0.05 - 10 Msun : HR tracks + times [CO-2e Fig 12.9] (Wuchterl & Tscharnuter 2003)

• Pre-Main Sequence

  • Pre-MS, 1 - 15 Msun : HR tracks + times [CO-1e Fig 12.8 + Tab 12.1] (Iben 1965)
  • Pre-MS, 0.8 - 60 Msun : HR tracks [CO-2e Fig 12.11] + times [CO-2e Tab 12.1] (Bernasconi & Maeder 1996)

• Post-Main Sequence

  • Post-MS, 1 Msun : HR track schematic [CO-2e Fig 13.4] (Caroll & Ostlie 2005)
  • AGB + Post-AGB, 0.6 Msun : HR track [CO-1e Fig 13.13; also CO-2e Fig 13.12] (Iben 1982)
  • Post-MS, 5 Msun : HR track schematic [CO-2e Fig 13.5] (Caroll & Ostlie 2005)
  • Post-MS, 5 Msun : HR track [CO-1e Fig 13.4] (Iben 1967)
  • Post-MS, 5 Msun : interior struct vs. time [CO-1e Fig 13.5] (Kippenhah et al. 1965)
  • Post-MS, 15 Msun : HR track [CO-1e Fig 13.15] (Woosley & Weaver 1986)
  • Post-MS, 1 - 15 Msun : HR tracks [CO-1e Fig 13.1] + times [CO-1e Tab 13.1] (Iben 1967)
  • Post-MS, 1 - 25 Msun : HR tracks [CO-2e Fig 13.1] + times [CO-2e Tab 13.1] (Schaller et al. 1992)
  • Post-MS, 9 - 120 Msun : HR tracks [CO-2e Fig 15.03] (Meynet & Maeder 2003)
  • Post-MS, 0.1 Msun : HR track [L97 Fig 1] (Laughlin et al. 1997)
  • Post-MS, 0.06 - 0.25 Msun : HR track [L97 Fig 2] (Laughlin et al. 1997)
  • Post-MS, 0.06 - 0.25 MSun : core ρ, T evolution vs. M, κ, R [L97 Fig 6] (Laughlin et al. 1997)

• Cluster Evolution

  • M3 globular cluster, age ~ 8-11 Gyr : CMD [CO-1e Fig 13.27; also CO-2e Fig 13.17] (Renzini & Fussi Pecci 1988)
  • h + χ Per "double" open cluster, age 14 Myr : CMD [CO-1e Fig 13.28; also CO-2e Fig 13.18] (Wildey 1964)
  • Many clusters w/ MS turnoffs : CMD [CO-1e Fig 13.29; also CO-2e Fig 13.19] (after Sandage)

• Pulsating Stars

  • Post-MS and Pulsating Stars, 1 - 25 Msun : HR tracks [CO-2e Fig 14.08] (Schaller et al. 1992)