Far-ultraviolet observations of the globular cluster 47 Tucanae

Details Far-ultraviolet observations of the globular cluster 47 Tucanae Far-ultraviolet observations of the globular cluster 47 Tucanae

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....52...59d&link_type=abstract

Astronomy and Astrophysics, vol. 52, no. 1, Oct. 1976, p. 59-62. Research sponsored by the Koninklijke Nederlandse Akademie van

Astronomy and Astrophysics

Astronomy

16

Far Ultraviolet Radiation, Globular Clusters, Ultraviolet Photometry, A Stars, Astronomical Netherlands Satellite, B Stars, Brightness, Spaceborne Astronomy, Spectral Bands, Spectral Energy Distribution

Scientific paper

Observations of 47 Tuc in five bands between 1550 and 3300 A by the Astronomical Netherlands Satellite are presented. The brightness distribution at 2200 and 3300 A agrees well with that in U; the color index C22-33 does not vary with radius. The excess flux between 1550 and 2500 A, observed at one position, is attributed to the B 8 III star in the cluster; the ultraviolet observations indicate a spectral type around A 0.

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