Photometry of occultation candidate stars. II - Uranus 1985-1990 and Saturn 1986-1991

Details Photometry of occultation candidate stars. II - Uranus 1985-1990 and Saturn 1986-1991 Photometry of occultation candidate stars. II - Uranus 1985-1990 and Saturn 1986-1991

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986icar...67..540f&link_type=abstract

Icarus (ISSN 0019-1035), vol. 67, Sept. 1986, p. 540-542.

Physics

4

Saturn Rings, Stellar Occultation, Stellar Spectrophotometry, Uranus Rings, Extremely High Frequencies, Interstellar Extinction, Stellar Color, Stellar Magnitude

Scientific paper

K magnitudes are given for seven Uranus-occulted stars, together with V and I magnitudes for 20 stars that will be occulted by the Uranian rings in 1986-1990 and 15 that will be occulted by the rings of Saturn in the course of 1986-1991. Occultation stars are noted to be up to 1 mag brighter in the K bandpass than could be predicted on the basis of V-I colors alone; this is explainable in terms of typical degrees of interstellar reddening.

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