Lizard
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- Understanding drop in luminosity during mass loss in HR diagram.
I am trying to understand the red line in the below diagram. This is Case B mass transfer (on a thermal timescale, through Roche-Lobe overflow).
Mass transfer begins at point B. Because this is mass transfer on a thermal timescale, it must be dynamically stable, meaning that the radius of the donor star must initially shrink in response to mass loss. However, I don't quite understand what is happening on the thermal timescale.
The first thing I don't understand is why the luminosity drops from point B to point C. It seems like this must be due to expansion from a perturbation to thermal equilibrium, but I don't understand why expansion is the response to mass loss.
The second thing I don't understand is why luminosity increases from point C to point D. The star reaches its maximum mass-loss rate at point C. Why would a decrease in mass loss rate result in an increase in luminosity? Why don't the arguments that describe the decrease in luminosity from B to C apply from C to D?
Mass transfer begins at point B. Because this is mass transfer on a thermal timescale, it must be dynamically stable, meaning that the radius of the donor star must initially shrink in response to mass loss. However, I don't quite understand what is happening on the thermal timescale.
The first thing I don't understand is why the luminosity drops from point B to point C. It seems like this must be due to expansion from a perturbation to thermal equilibrium, but I don't understand why expansion is the response to mass loss.
The second thing I don't understand is why luminosity increases from point C to point D. The star reaches its maximum mass-loss rate at point C. Why would a decrease in mass loss rate result in an increase in luminosity? Why don't the arguments that describe the decrease in luminosity from B to C apply from C to D?
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