Apollo 17 far-ultraviolet spectra in the Large Magellanic Cloud

Details Apollo 17 far-ultraviolet spectra in the Large Magellanic Cloud Apollo 17 far-ultraviolet spectra in the Large Magellanic Cloud

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....53..317h&link_type=abstract

Astronomy and Astrophysics, vol. 53, no. 2, Dec. 1976, p. 317-319.

Astronomy and Astrophysics

Astronomy

6

Apollo 17 Flight, Far Ultraviolet Radiation, Magellanic Clouds, Spaceborne Astronomy, Ultraviolet Spectra, Astronomical Spectroscopy, B Stars, Interstellar Extinction, O Stars, Ultraviolet Spectroscopy

Scientific paper

During the Apollo 17 mission, low-resolution far-ultraviolet spectra
were obtained for two parts of the Large Magellanic Cloud. The spectra
are reasonably well fit by a model of a 30,000-K star reddened by a
(B-V) color excess of 0.3 magnitude, but other combinations of
temperature and reddening provide equally good fits.

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