Some physical mechanisms which can affect the Zeeman line profiles of magnetic white dwarfs are studied. The pure absorption polarization transfer equation is solved including these mechanisms. The broadening of lines in magnetic white dwarfs is briefly discussed, Es werden physikalische Mechanismen
โฆ LIBER โฆ
Line formation in white dwarf atmospheres
โ Scribed by F. Allard; R. Wehrse
- Publisher
- Elsevier Science
- Year
- 1990
- Tongue
- English
- Weight
- 401 KB
- Volume
- 44
- Category
- Article
- ISSN
- 0022-4073
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