Free Access
Volume 542, June 2012
Article Number A113
Number of page(s) 29
Section Stellar structure and evolution
Published online 19 June 2012

Online material

Table 3

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.

Table 4

Yields of stellar winds from rotating models, in units of solar mass.

Table 5

Yields in the last calculated model for each model sequence, in units of solar mass.

Appendix A: Kippenhan diagram

thumbnail Fig. A.1

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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