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Absorption Lines of Call and H in the Near IR Region of the Magnetic Star HD 152107
Published online by Cambridge University Press: 12 April 2016
Abstract
A behaviour of H lines P12 - P13 and CaII triplet of the star HD 152107 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.
- Type
- Section III - Magnetic CP Stars
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- Copyright © Reidel 1986