This test case checks that the evolution of a 7 Msun, metal-poor Z = 0.001, model reaches the AGB.
This test case has two parts. Click to see a larger view of a plot.
- Part 1 (
inlist_start) creates a pre-main sequence model.
- Part 2 (
inlist_7M_prems_to_AGB) continues the evolution as core hydrogen and helium burning proceed, terminating when log10(L/Lsun)=4.3 is reached. The model executes a blue loop as helium depletes, with the red edge and blue edge of the classical Cepheid instability strip boundaries shown in the HR diagram:
pgstar commands used:
&pgstar file_white_on_black_flag = .true. ! white_on_black flags -- true means white foreground color on black background file_device = 'png' ! png file_extension = 'png' !file_device = 'vcps' ! postscript !file_extension = 'ps' pgstar_interval = 10 HR_win_flag = .true. HR_win_width = 12 HR_win_aspect_ratio = 1.2 ! aspect_ratio = height/width HR_logT_min = 3.5 HR_logT_max = 4.5 HR_logL_min = 2.7 HR_logL_max = 4.4 ! file output HR_file_flag = .true. HR_file_dir = 'pgstar_out' HR_file_prefix = 'hr' HR_file_interval = 100 ! output when mod(model_number,HR_file_interval)==0 HR_file_width = 15 ! negative means use same value as for window HR_file_aspect_ratio = -1 ! negative means use same value as for window / ! end of pgstar namelist
Last-Updated: 29May2021 (MESA e37f76f) by fxt