Photometry of occultation candidate stars. II. Uranus 1985-1990 and Saturn 1986-1991
- Linda M. French(corresponding author),
- Guarionex Morales,
- Steven L. Gaiser,
- Jay A. Frogel
- Massachusetts Institute of Technology,
- Kitt Peak National Observatory
Scholarship:
Journal Article
Article
Peer-reviewAbstract
V and I magnitudes are presented for 20 stars to be occulted by the Uranian rings during the period 1986-1990 and for 15 stars to be occulted by Saturn's rings during 1986-1991. K magnitudes for seven Uranus stars are presented. The occultation stars are up to one magnitude brighter in the K bandpass than one would predict on the basis of V-I colors alone. This effect can be explained by typical amounts of interstellar reddening.
Scholarship
Output type
Scholarship:
Journal Article
Article
Peer-reviewOriginal language
EnglishPages from-to (Number of pages)
Pages 540-542 (3 pages)Journal (Volume, Issue Number)
Icarus (Volume 67, Issue 3)Publication milestones
- Published - 09/1986
Publication status
Published - 09/1986
ISSN
0019-1035Publication IDs
- Scopus: 46149129595
Funding Details
This work was supportedby NASA Grant NSG-7526a nd NSF Grant AST-8209825.W e thankO scar Rivera fora ssistancaet the telescopaet CTIO, and GabrieMl enchacfao r the preparatoiofn fi nderc harts. We also gratefullya cknowledgteh e supporotf the MIT UndergraduaRtee searcOh pportunitiePsr ogram.
FundersFunding number
NSF
AST-8209825
NASA
-