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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

T.N. Kuznetsova
T.N. Kuznetsova*
Affiliation:
The USSR Academy of Sciences Central Astronomical observatory at Pulkovo 196140 Leningrad, USSR

Abstract

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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
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 323 - 326
Copyright
Copyright © Reidel 1986

References

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