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- W129424025 abstract "The existence of a group of magnetic white dwarfs with mean surface fields of between ~5 × 10 6 G and ~2 × 1O 7 G is now firmly established through the discovery of Zeeman structure in hydrogen and helium lines (Angel et al . 1974, Liebert et al . 1975, Wickramasinghe et al . 1977, Martin & Wickramasinghe 1978, Liebert et al . 1977). There is considerable evidence from polarimetric studies for even higher fields in some white dwarfs (Angel 1977). Most of these stars are cool and show nearly continuous spectra or weak unidentified absorption features. The possibility of cyclotron absorption in white dwarfs was first discussed in connection with the infrared polarisation spectrum of one of these stars, Grw + 70°8247 (Kemp 1970). More recently the polarised white dwarf GD229 was found to have a rich optical spectrum with a strong feature at λ4185, for which cyclotron absorption has been mentioned as a possible origin (Angel 1977, Greenstein & Boksenberg 1977), though without supporting computations. In this letter we use models to investigate this possibility further." @default.
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- W129424025 date "1978-01-01" @default.
- W129424025 modified "2023-10-18" @default.
- W129424025 title "Cyclotron Absorption in GD229?" @default.
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- W129424025 doi "https://doi.org/10.1017/s1323358000015514" @default.
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