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- W1972382238 abstract "The ultraviolet spectrum of Arcturus has been observed at high resolution with the IUE satellite. Line identifications, mean absolute 'continuum' flux measurements, integrated absolute emission-line fluxes, and measurements of selected absorption line strengths are presented for the 2250-2930 A region. In the 1150-2000 A region, identifications are given primarily on the basis of low-resolution spectra. Chromospheric emission lines have been identified with low-excitation species including H I, C I, C II, O I, Mg I, Mg II, Al II, Si I, Si II, S I, and Fe II; there is no evidence for lines of C IV, N V, or other species requiring high temperatures. A search for molecular absorption features in the 2500-2930 A interval has led to several tentative identifications, but only OH could be established as definitely present. Iron lines strongly dominate the identifications in the 2250-2930 A region, Fe II accounting for about 86 percent of the emission features and Fe I for 43 percent of the identified absorption features." @default.
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- W1972382238 date "1985-02-01" @default.
- W1972382238 modified "2023-09-23" @default.
- W1972382238 title "Line identifications, line strengths, and continuum flux measurements in the ultraviolet spectrum of Arcturus" @default.
- W1972382238 doi "https://doi.org/10.1086/191009" @default.
- W1972382238 hasPublicationYear "1985" @default.
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