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ICCD Speckle Observations of Binary Stars.XV.An Investigation of Lunar Occultation Systems Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1996AJ....112.2260M&db_key=AST
| E. W. Fick Observatory stellar radial velocity measurements. I - 1976-1984 Stellar radial velocity observations made with the large vacuumhigh-dispersion photoelectric radial velocity spectrometer at FickObservatory are reported. This includes nearly 2000 late-type starsobserved during 585 nights. Gradual modifications to this instrumentover its first eight years of operation have reduced the observationalerror for high-quality dip observations to + or - 0.8 km/s.
| Binary stars unresolved by speckle interferometry. III The KPNO's 4-m telescope was used in 1975-1981 to determine the epochsof 1164 speckle observations for 469 unresolved, known or suspectedbinary stars. The data, presented in tabular form, encompass visualbinaries with eccentric orbits, occultation binaries, astrometricbinaries, Hyades stars of known or suspected duplicity, and many longperiod spectroscopic binaries.
| Photoelectric observations of lunar occultations. X Photoelectric occulation results for 461 events observed during 15months are reported. They include 77 reappearances, 4 determinations ofangular diameter, 38 analyses of double or multiple stars including twopreviously unknown bright stars, and 8 previously known bright double ormultiple stars.
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Observation and Astrometry data
Constellation: | Balance |
Right ascension: | 15h11m49.98s |
Declination: | -16°09'34.4" |
Apparent magnitude: | 6.678 |
Distance: | 137.931 parsecs |
Proper motion RA: | -11.7 |
Proper motion Dec: | -21.4 |
B-T magnitude: | 8.324 |
V-T magnitude: | 6.814 |
Catalogs and designations:
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