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The Most Iron-Deficient Manganese Star HR562
Published online by Cambridge University Press: 12 April 2016
Abstract
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Abundances of 11 elements are determined in the atmosphere of the manganese star HR562 = HD11905 (B8III, Te = 14000 K, log g=3.5). The deficit of iron of 0.9 dex is extreme among HgMn stars. The excess of mercury abundance amounts to 4.8 dex.
- Type
- Section IV - Non-Magnetic CP and Related Stars
- Information
- Copyright
- Copyright © Reidel 1986
References
Cowley, C.R., Sears, R.L., Aikraan, G.C.L., and Sadakane, K.
1982, Ap. J., 254, 191.CrossRefGoogle Scholar
Kurucz, R.L., Peytremann, E., and Avrett, E.H.
1974, Blanketed Model Atmospheres for Early-type Stars, (Washington: Smithsonian Inst.).Google Scholar
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