The atmosphere of the hydrogen-deficient star sigma Orionis E
Sigma Orionis E hydrogen-deficient atmosphere, using grid of constant-flux model atmospheres to determine abundances of five elements
Bless, R. C.↗
Engineering topics
Publications and source records attributed to Klinglesmith, D. A..
Sigma Orionis E hydrogen-deficient atmosphere, using grid of constant-flux model atmospheres to determine abundances of five elements
Nonlinear limb darkening for early stars
Hydrogen abundance in white dwarfs, discussing inconsistencies in mass and bolometric magnitude models for Sirius and Eri B
Carbon content of helium star from coude spectrograms analysis based on flux constant model atmospheres