The Rosseland mean opacity of stellar atmospheres

Details The Rosseland mean opacity of stellar atmospheres The Rosseland mean opacity of stellar atmospheres

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982cha%26a...6...20j&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 6, Issue 1, p. 20-23.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Rosseland mean opacities āR(T,lgPe) [see Table 2] per unit hydrogen particle are calculated in this paper for the atmosphere of the solar type [see Table 1].
The sources of the continuous opacities under consideration in this paper are as follows: (1) H-, HI, H-2, H+2 He-, HeI, HeII, CI, CII, CIII, NI, NII, NIII, OI, OII, NaI, MgI, MgII, AlI, AlII, SiI, SiII, CII, KI, CaII in the form of absorption. (2) HI, HeI, CI, NI, OI, H2 in the form of Rayleigh scattering. (3) Free electrons in the form of Thomson scattering.

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