Abstract
A behaviour of H lines P12 - P18 and CaII triplet of the star HD I52I07 is studied in the range λλ 8400 – 8800 Å. An analysis of the obtained data enabled us to suspect the presence of a relationship between the variation of equivalent widths of the lines of the Paschen series of Hydrogen CaII lines and that of the star’s magnetic field.
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© 1986 D. Reidel Publishing Company
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Kuznetsova, T.N. (1986). Absorption Lines of CaII and H in the Near IR Region of the Magnetic Star HD 152107. 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_51
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DOI: https://doi.org/10.1007/978-94-009-4714-6_51
Publisher Name: Springer, Dordrecht
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