EDP Sciences
Free Access
Issue
A&A
Volume 581, September 2015
Article Number A15
Number of page(s) 35
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/201526617
Published online 25 August 2015

Online material

Appendix A: Key quantities of our model sequences

Table A.1

Important characteristics of our models.

Appendix B: Photoionising flux

Table B.1

Time averaged ionising fluxes (L), and time averaged (Q) and peak photon emission rates (Qmax) of the ionising photons for hydrogen (H), neutral helium (He) and singly ionised helium (He+) during the main-sequence evolution for each stellar sequence.

Appendix C: Isochrones

Figure C.1 shows isochrones of our stellar evolutionary calculations for several ages and rotational rates.

thumbnail Fig. C.1

Isochrones of different ages of rotating stellar evolutionary models are shown in the HR diagram. The initial surface rotational velocity is chosen in steps of 100 km s-1 from non-rotating to 600 km s-1.

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© ESO, 2015

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