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- W3027673818 abstract "AM Herculis stars form a subclass of cataclysmic variables, the defining characteristic of which is that they possess a high degree of polarisation at optical frequencies. Physically they have two notable features. Firstly, the white dwarf star has a sufficiently high magnetic field (B ~ 10." @default.
- W3027673818 created "2020-05-29" @default.
- W3027673818 creator A5081804398 @default.
- W3027673818 date "1986-01-01" @default.
- W3027673818 modified "2023-09-23" @default.
- W3027673818 title "Energy Transport in Radially Accreting White Dwarf Stars" @default.
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