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- W1581268917 abstract "There are some 30 white dwarfs which are known to be magnetic with fields in the range 106–109 Gauss. A somewhat smaller number are found in the close interacting binary systems known as the AM Herculis variables. We discuss how Zeeman and cyclotron spectroscopy have been used to determine fields and study fields structure in these stars." @default.
- W1581268917 created "2016-06-24" @default.
- W1581268917 creator A5052077765 @default.
- W1581268917 date "1990-01-01" @default.
- W1581268917 modified "2023-09-24" @default.
- W1581268917 title "Zeeman and cyclotron lines from magnetic white dwarfs" @default.
- W1581268917 doi "https://doi.org/10.1063/1.39866" @default.
- W1581268917 hasPublicationYear "1990" @default.
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