Fitting Atmospheres to Stars
نویسندگان
چکیده
منابع مشابه
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Using a Hartree-Fock formalism, we estimate energy levels and photon cross sections for atomic iron in magnetic Ðelds BD 1013 G. Computing ionization equilibrium and normal mode opacities with these data, we construct LTE neutron star model atmospheres at 5.5 \ log and compute emergent (Teff) \ 6.5 spectra. We examine the dependence of the emergent spectra on and B. We also show the spectral Te...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1938
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/98.3.199