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The Magnetic Field and other Parameters of the Chemically Peculiar Stars

Published online by Cambridge University Press:  12 April 2016

Glagolevskij Yu.V. ,
Romanyuk I.I.  and
Chunakova N.M.
Glagolevskij Yu.V.
Affiliation:
Special Astrophysical Observatory Stavropolskij Kraj Ni znij Arkhyz 357147, USSR
Romanyuk I.I.
Affiliation:
Special Astrophysical Observatory Stavropolskij Kraj Ni znij Arkhyz 357147, USSR
Chunakova N.M.
Affiliation:
Special Astrophysical Observatory Stavropolskij Kraj Ni znij Arkhyz 357147, USSR

Abstract

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The surface field Bs ( but not the effective Be one ) is responsible for different processes occuring in the magnetic stars atmospheres. For this reason it is natural that different investigators are interested in working out and improving methods of determination of Bs. Especially great attention attracts the method based on using the multicolor Geneva photometry. Cramer and Maeder have found a dependence between Bs and parameter Z of multicolor photometry wich they use for the estimation of the surface field. But it is necessary to investigate this method before application. Due to this reason we have put the following two problems:

A - The search for stars with a maximal predicted field

B - Examination of calibration of Bs (Z).

Type
Section I - Theoretical Considerations
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 33 - 36
Copyright
Copyright © Reidel 1986

References

1. Cramer, N., Maeder, A., Astron. Astrophys. Suppl. Ser., 1980, v. 41, p. 111 – 115.Google Scholar
2. Brown, D.N., Landstreet, J.D., Thompson, I. Upper main sequence, 23-d Liege Coll., Liege, 1981, p.195 – 198.Google Scholar
3. Fleck, R.C., Upper main sequence, 23-d Liege Coll., Liege, 1981,p.341 – 342.Google Scholar