Volume 542, June 2012
|Number of page(s)||29|
|Section||Stellar structure and evolution|
|Published online||19 June 2012|
Total energy (E), total number (N), and average wavelength () of the ionizing photons for hydrogen (H), neutral helium (He) and singly ionized helium (He+) during the evolution for each model sequence.
Yields of stellar winds from rotating models, in units of solar mass.
Yields in the last calculated model for each model sequence, in units of solar mass.
Kippenhahn diagram for different model sequences. The sequence number is shown in each diagram. Convective and overshooting layers are marked by green and yellow hatched lines, respectively. Semi-convective layers are marked by red dots. The net amount of energy loss and gain is indicated by color shading. The surface of the star is marked by a black solid line.
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© ESO, 2012
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