Fe II in the International Ultraviolet Explorer (IUE) spectra of emission line stars

Details Fe II in the International Ultraviolet Explorer (IUE) spectra of emission line stars Fe II in the International Ultraviolet Explorer (IUE) spectra of emission line stars

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157...39v&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

4

Emission Spectra, Iron, Iue, Stellar Spectra, Ultraviolet Astronomy, Absorption Spectra, Atomic Excitations, Ions, Magellanic Clouds, Optical Thickness

Scientific paper

The behavior of the Fe II lines in the ultraviolet spectra of the emission line stars Boss 1985, eta Car, and S 22 in the Large Magellanic Cloud was examined. The dependence of the Fe II line emission as a function of the excitation potential, line strength, and wavelength is discussed. Increased optical thickness of the emission lines, the presence of absorption components, and in many cases, a large negative continuum gradient make the study of Fe II in low resolution spectra more difficult.

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