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The Quadratic Zeeman Effect for CI Lines-Application to the Spectrum of EG 129

Published online by Cambridge University Press:  12 April 2016

I. Bues  and
G. Varvatis
I. Bues
Affiliation:
I. Mathem. Inst. Freie Universität Berlin F.R.G.
G. Varvatis
Affiliation:
I. Mathem. Inst. Freie Universität Berlin F.R.G.

Extract

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Garstang and Kemic (1974) derived formulae for the splitting of hydrogen and helium lines in the presence of large magnetic fields. We applied their method in calculating the eigenvectors for some transitions of neutral carbon, where a correction factor for the coupling and mixing of the energy levels has to be applied. For CI – lines in the visible region of the spectrum, well separated components can be expected for a field strength up to 2 • 107G. Fig. 1 shows the splitting of three lines for B = 107 G.

Type
Colloquium Session V
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 322 - 323
Copyright
Copyright © The University of Rochester 1979

References

Garstang, R.H., Kemic, S.B. 1974, Astrophys. Space Sc. 31, 103.CrossRefGoogle Scholar