imf - cosmos.phy.tufts.educosmos.phy.tufts.edu/~danilo/ast121/material/lecturefigures_20_25.pdf ·...
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![Page 1: IMF - cosmos.phy.tufts.educosmos.phy.tufts.edu/~danilo/AST121/Material/LectureFigures_20_25.pdf · To white dwarf phase Logw(Te) FIGURE 13.4 A schematic diagram oftheevolutionof a](https://reader031.vdocuments.us/reader031/viewer/2022030402/5a78ee7d7f8b9a70238e97e8/html5/thumbnails/1.jpg)
IMF
![Page 2: IMF - cosmos.phy.tufts.educosmos.phy.tufts.edu/~danilo/AST121/Material/LectureFigures_20_25.pdf · To white dwarf phase Logw(Te) FIGURE 13.4 A schematic diagram oftheevolutionof a](https://reader031.vdocuments.us/reader031/viewer/2022030402/5a78ee7d7f8b9a70238e97e8/html5/thumbnails/2.jpg)
![Page 3: IMF - cosmos.phy.tufts.educosmos.phy.tufts.edu/~danilo/AST121/Material/LectureFigures_20_25.pdf · To white dwarf phase Logw(Te) FIGURE 13.4 A schematic diagram oftheevolutionof a](https://reader031.vdocuments.us/reader031/viewer/2022030402/5a78ee7d7f8b9a70238e97e8/html5/thumbnails/3.jpg)
![Page 4: IMF - cosmos.phy.tufts.educosmos.phy.tufts.edu/~danilo/AST121/Material/LectureFigures_20_25.pdf · To white dwarf phase Logw(Te) FIGURE 13.4 A schematic diagram oftheevolutionof a](https://reader031.vdocuments.us/reader031/viewer/2022030402/5a78ee7d7f8b9a70238e97e8/html5/thumbnails/4.jpg)
![Page 5: IMF - cosmos.phy.tufts.educosmos.phy.tufts.edu/~danilo/AST121/Material/LectureFigures_20_25.pdf · To white dwarf phase Logw(Te) FIGURE 13.4 A schematic diagram oftheevolutionof a](https://reader031.vdocuments.us/reader031/viewer/2022030402/5a78ee7d7f8b9a70238e97e8/html5/thumbnails/5.jpg)
D burning
Envelope becomes radiative
Core becomes convective
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M~0.8 MsunM~1 Msun
M~2 Msun
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M/Msun<0.8
0.8<M/Msun<2
M/Msun>2
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5 Msun star with He core and H-burning shell shortly after shell ignition
5 Msun star on the early asymptotic giant branch with C-O core and H- and He-burning shells. The scale of the shells and core has been increased by x100.
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M3, old globular cluster
MS
TO
BS
P-AGB
HB
AGB
RGB
SGB
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