Abundances - for X-ray opacities - summary July 28, 2010 D. Cohen Abundances (and even moreso, overall metallicity) are the biggest uncertainty in modeling the wind opacity in the x-ray regime. Ionization balance makes a small difference, but quite small (He-recombination in the outer wind aside - and so we generally use a "standard O star" mix of ionization stages). The big issues, then, for making an appropriate model of the X-ray opacity for a given star are: 1. Which solar abundances? and 2. Are specific elements (esp. CNO) altered from their solar values? Note that for normal O stars in the Galaxy, there's little evidence for deviations from overall solar metallicity (though specific CNO abundances generally don't sum to the solar value - though the solar value is generally within the systematic uncertainties on these determinations). log 12 (H) scale: AGS05 Aspl09 He 10.93 10.98 C 8.39 8.47 N 7.78 7.87 O 8.66 8.73 Ne 7.84 7.97 Mg 7.53 7.64 Si 7.51 7.55 Fe 7.45 7.54 From Taresch et al. for HD 93129A (assuming their values are scaled to GS89 and then rescaling them to Aspl09): Y_C = 0.25 Y_N = 3.02 Y_O = 0.47 Note that the sum of C, N, and O totals to 0.68 of Aspl09 solar These are the values used for Maurice's opacity model (July 2010): kappa.HD93129A.CNOsubsolar.fits 12 Aug 2010: And we have a "HD93129A.CNOsolar" version too, in which we scale up the C, N, and O abundances by 1/0.68 so that their sum is solar, giving individual abundances of: Y_C = 0.37 Y_N = 4.44 Y_O = 0.69 ---- List of opacity files available for use with windtabs or for analyzing taustar --> Mdot --- kappa_ags_zp_alt1 = CNO processed, solar (AGS05) metallicity; CNO rescaled back up to solar (in sum) kappa_aspl09 = Asplund 09 solar abund w/ standard ion mix kappa_solarAGS05 = Asplund Gr. Sau. 05 solar abunda w/ different(?) ion mix kappa.HD93129A.CNOsubsolar.dat = asp09 metallicity, w/ CNO altered acc. to Taresch; standard ion mix kappa.HD93129A.CNOsolar.dat = asp09 metallicity, w/ CNO altered acc. to Taresch, but then rescaled so sum of C, N, and O = solar. (T.'s determination gives 0.68 solar)