Hydrogen-deficient Model Atmospheres for Degenerate Stars |
Contents
THE COMPUTATION OF THE MODEL STELLAR ATMOSPHERES | 15 |
LINE PROFILE COMPUTATION | 47 |
MODELS FOR THE 4670 STARS | 61 |
3 other sections not shown
Common terms and phrases
absorption coefficient abundance allows APPENDIX approximation atomic carbon blend broadening C2 Swan bands CaII calculation Call carbon-rich chapter colors complete composition computed constant continuum convective flux Convective Models cool correction corresponding Curves degeneracy degenerate stars density discussed effective temperature electron energy equation equilibrium equivalent width errors Figure formulae four frequency function given gives gram helium hydrogen lines included increase indicate integration intensity interpolation ionized iteration layers length less line profiles line-blanketed models lower Maanen magnitude mass mean metal method Mihalas model atmosphere molecular molecules neutral observed obtained opacity opacity source optical depth parameters plane polynomial pressure radiation radiative models range ratio region relation relative rotational scattering shows solve source function spectral Stark stellar step Swan bands Teff temperature distribution tion transition unblanketed unit values vibrational wavelength