Comparison of UV spectra from solar-type stars

Details Comparison of UV spectra from solar-type stars Comparison of UV spectra from solar-type stars

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...94....3g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 94, Aug. 1984, p. 3-11.

Astronomy and Astrophysics

Astronomy

4

Solar Spectra, Stellar Spectra, Ultraviolet Astronomy, Ultraviolet Spectra, Comparison, Iue, Late Stars, Line Spectra, Magnesium, Spectrum Analysis

Scientific paper

The authors compare high-resolution spectra from the Sun and the four solar-type stars 16 Cyg A, 16 Cyg B, HD 32008, HD 34411 obtained with IUE in the wavelength range 2650-2930 Å. The comparison is made for peak intensities between absorption lines. At the level of accuracy of the IUE observations, the stars 16 Cyg A, 16 Cyg B, HD 34411 are indistinguishable from the Sun, in particular the Mg II resonance line profiles are identical. HD 32008 is not a solar analog but is evidently of late G to early K spectral type.

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