Mariner 9 Ultraviolet Spectrometer Experiment: Stellar Observations

Details Mariner 9 Ultraviolet Spectrometer Experiment: Stellar Observations Mariner 9 Ultraviolet Spectrometer Experiment: Stellar Observations

Jan 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972sci...175..321l&link_type=abstract

Science, Volume 175, Issue 4019, pp. 321-322

Physics

7

Scientific paper

Photoelectric spectra have been obtained for a number of early-type stars in the 1100- to 2000-angstrom region with the Mariner 9 ultraviolet spectrometer. The resonance lines of H I, Si IV, and C IV are easily identified, as are features due to C II, C III, Si III, Fe II, N IV. The absolute energy distribution derived from the data lie about 20 percent below those of OAO-2 in the 1200- to 2000-angstrom region.

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