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Abundance Analysis of Three Ap Stars: Hd2453, Hd8441, and Hd192913

Published online by Cambridge University Press:  12 April 2016

T.A. Ryabchikova  and
D.A. Ptitsyn
T.A. Ryabchikova
Affiliation:
The Astronomical Council of the U.S.S.R. Academy of Sciences Pyatnitskaya Str. 48, Moscow 109017, U.S.S.R.
D.A. Ptitsyn
Affiliation:
The Astronomical Council of the U.S.S.R. Academy of Sciences Pyatnitskaya Str. 48, Moscow 109017, U.S.S.R.

Abstract

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Using 9 Å/mm-dispersion spectra of two Ap stars (HD2453 and HD8441) from the list by Adelman (1973) and the SiCr star HD192913 the abundances of 19 elements are obtained by the model atmosphere technique. The curve-of-growth method is used to estimate the surface magnetic field from Fe, Cr, and Ti lines.

Type
Section III - Magnetic CP Stars
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 319 - 322
Copyright
Copyright © Reidel 1986

References

Adelman, S.J. 1973, Ap. J. Suppl. 26, 1.Google Scholar
Adelman, S.J. 1984, Astr. Ap., 141, 362.Google Scholar
Grevesse, N. 1984, Phys. Scripta, T8, 49.Google Scholar
Kurucz, R.L., Peytremann, E., and Avrett, E.H. 1974, Blanketed Model Atmospheres for Early-Type Stars (Washington: Smithsonian Inst.).Google Scholar
Landi Degl’Innocenti, E. 1975, Astr. Ap., 45, 269.Google Scholar
Piskunovv, N.E., Ptitsyn, D.A., Ryabchikova, T.A., and Khokhlova, V.L. 1984, Nauchnye Informatali, Astr. Sovet Akademii Nauk SSSR, 54, 45.Google Scholar
Ryabchikova, T.A., and Piskunov, N.E. 1984, in: Magnetic Stars, Proc. Conf. held in Riga, April 10-12, 1984, ed. Khokhlova, V., Ptitsyn, D., and Lielausis, O. (Salaspils: Latvian Phys. Inst.), p. 59.Google Scholar