Abstract
We analyze IUE spectra of the star 1016 Ori. Together with previously obtained visible spectra, they have allowed the wavelength range from 1150 to 7000 Å to be studied. Atmospheric parameters of the star were refined: logg=4.5(1), T eff=30000(1000) K, and ξt=15(5) km s−1. We measured the equivalent widths of ∼500 lines and used them to compute the chemical composition. It turned out that the He, B, Mg, P, and S abundances were nearly solar; Ne, Ti, and Cr were overabundant; and C, N, O, Al, Si, Mn, Fe, Ni, and Zn were underabundant.
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Translated from Pis’ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 27, No. 12, 2001, pp. 940–947.
Original Russian Text Copyright © 2001 by Vitrichenko.
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Vitrichenko, É.A. Analysis of IUE spectra for the star V1016 Ori. Astron. Lett. 27, 809–815 (2001). https://doi.org/10.1134/1.1424364
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DOI: https://doi.org/10.1134/1.1424364