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High dispersion IUE spectra of active chromosphere G and K dwarfs

T. R. Ayres, Jeffrey L. Linsky, A. M. Brown, C. Jordan, T. Simon

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Abstract

IUE far ultraviolet echelle spectra of three active chromosphere dwarf stars X1 Orionis (GO V), Bootis A (G8 V), and Eridani (K2 V), are analyzed utilizing spectra of Alpha Cen A (G2 V) and Alpha Cen B (K1 V) as quiet chromosphere comparisons.

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What this paper is about

IUE far ultraviolet echelle spectra of three active chromosphere dwarf stars X1 Orionis (GO V), Bootis A (G8 V), and Eridani (K2 V), are analyzed utilizing spectra of Alpha Cen A (G2 V) and Alpha Cen B (K1 V) as quiet chromosphere comparisons.

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Available abstract

IUE far ultraviolet echelle spectra of three active chromosphere dwarf stars X1 Orionis (GO V), Bootis A (G8 V), and Eridani (K2 V), are analyzed utilizing spectra of Alpha Cen A (G2 V) and Alpha Cen B (K1 V) as quiet chromosphere comparisons.

Key concepts: Chromosphere, Physics, Astrophysics, Spectral line, Ultraviolet astronomy, Stars, Astronomy, Stellar classification

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