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Computation of convective model atmospheres of cool white dwarfs

✍ Scribed by A. Galdikas


Publisher
Springer Netherlands
Year
1984
Tongue
English
Weight
284 KB
Volume
105
Category
Article
ISSN
0004-640X

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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