New Results on Radiative Forces on Iron in Hot White Dwarfs
- 1 January 1991
- book chapter
- Published by Springer Nature
Abstract
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This publication has 12 references indexed in Scilit:
- Heavy element abundances predicted by radiative support theory in the atmospheres of hot white dwarfsPublished by Springer Nature ,2008
- Ultraviolet Fe VII absorption lines in planetary nebula nuclei, hot subdwarfs, and hot degenerate objectsThe Astrophysical Journal, 1990
- Chemical separation in horizontal-branch starsThe Astrophysical Journal, 1983
- Energy Levels of Iron, Fe I Through Fe XXVIJournal of Physical and Chemical Reference Data, 1982
- Atomic transition probabilities for iron, cobalt, and nickel (A critical data compilation of allowed lines)Journal of Physical and Chemical Reference Data, 1981
- Diffusion time scales in white dwarfsThe Astrophysical Journal, 1979
- Equations of State for Stellar Partial Ionization ZonesThe Astrophysical Journal Supplement Series, 1977
- Diffusion in main-sequence stars - Radiation forces, time scales, anomaliesThe Astrophysical Journal, 1976
- Convective white-dwarf envelope model grids for H-, He-, and C-rich compositionsThe Astrophysical Journal Supplement Series, 1976
- Rosseland Opacity Tables for Population II CompositionsThe Astrophysical Journal Supplement Series, 1970