Graphs from Interior Code BZAMS3

Astronomy 421 Autumn 2006

Convection
0.5 Msun with emphasis on the upper layers 0.5 Msun vs [1 - m/M] where m/M represents the mass at a given grid point versus the total mass of the star
1 Msun with emphasis on the upper layers 1 Msun vs [1 - m/M] where m/M represents the mass at a given grid point versus the total mass of the star
2 Msun with emphasis on the upper layers 2 Msun vs [1 - m/M] where m/M represents the mass at a given grid point versus the total mass of the star
5 Msun with emphasis on the upper layers 5 Msun vs [1 - m/M] where m/M represents the mass at a given grid point versus the total mass of the star
10 Msun with emphasis on the upper layers 10 Msun vs [1 - m/M] where m/M represents the mass at a given grid point versus the total mass of the star
20 Msun with emphasis on the upper layers 20 Msun vs [1 - m/M] where m/M represents the mass at a given grid point versus the total mass of the star
Additional relationships among the different mass models
r/Rtot vs [1 - mM] (note: x-axis is reversed)
L/Ltot vs [1 - m/M]
log10(epsilon) vs [1 - m/M]
log10(density) vs [1 - m/M] log10(density) vs -log10(1 - m/M) emphasis on the upper layers
log10(pressure) vs [1 - m/M]
log10(temperature) vs [1 - m/M]
log10(T) vs -log10(1 - m/M) emphasis on the upper layers
log10(kappa) vs -log10(1 - m/M)
Excel Spreadsheets
bzams3.xls with graphs emphasizing upper layers