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Issue A&A
Volume 499, Number 1, May III 2009
Page(s) 279 - 290
Section Stellar structure and evolution
DOI http://dx.doi.org/10.1051/0004-6361/200911643
Published online 12 March 2009

Online Material

Appendix A: Models

Table A.1:   Outermost 4 $~{R}_\odot$ of a 60 $~{M}_\odot$ model at solar metallicity (Z=0.02). The table shows physical variables at t =  $2.37\times 10^6$years. Columns contain the progressive grid point of the model, the status ( $R=\rm radiative$, $C=\rm convective$), the optical depth $\tau $, the opacity $\varkappa $, the density $\rho $, the radius R, the value M*-Mr (where M* is the total stellar mass and Mr is the mass coordinate), the temperature T, the convective velocity $v_{\rm c}$ and the local sound speed $c_{\rm s}$. All the values are in cgs units if not otherwise specified.

Table A.2:   Outermost 1 $~{R}_\odot$ of a 20  $~{M}_\odot$ model at solar metallicity (Z=0.02). The table shows the physical variables at t =  $6.41\times 10^6$ years. Columns contain the progressive grid point of the model, the status (R = radiative, C = convective), the optical depth $\tau $, the opacity $\varkappa $, the density $\rho $, the radius R, the value M*-Mr (where M* is the total stellar mass and Mr is the mass coordinate), the temperature T, the convective velocity $v_{\rm c}$ and the local sound speed $c_{\rm s}$. All the values are in cgs units if not otherwise specified.





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