Abstract
In spectra of chemically peculiar (CP) stars the weak lines originate at very different levels on the both sides of the Balmer jump (λB = 3646 A): τ ≈ 0.01 at λ < 3646 Å and τ ≈ 0.5 – 1.0, when λ > 3646 Å (Khokhlova, 1978).
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© 1986 D. Reidel Publishing Company
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Romanyuk, I.I. (1986). Some Structural Features of Magnetic Fields of the Chemically Peculiar Stars β Cr B and α2CVn. In: Cowley, C.R., Dworetsky, M.M., Mégessier, C. (eds) Upper Main Sequence Stars with Anomalous Abundances. Astrophysics and Space Science Library, vol 125. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4714-6_58
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DOI: https://doi.org/10.1007/978-94-009-4714-6_58
Publisher Name: Springer, Dordrecht
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