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HD 96589


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Stromgren Four-Colour UVBY Photometry of G5-TYPE Hd-Stars Brighter than MV=8.6
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1993A&AS..102...89O&db_key=AST

Photometry of 50 suspected variable stars
Fifty stars have been chosen as suspected variable stars and analyzedfor variability. A large portion of this sample are stars that areeither proved active chromosphere stars or are candidates for suchactivity. The photometric data base consists of differential Vmeasurements of the Vanderbilt 16 inch (41 cm) automatic photoelectrictelescope and 25 observers at 26 observatories worldwide. Publishedphotometric data have also been utilized, with proper adjustments madeto ensure that all magnitudes are differential. Searches for photometricperiod, amplitudes, and times of minimum light showed 68 percent of thesample to be photometrically variable with periods found for 34. Twostars were deemed norvariable for the period of observation. Conclusivestatements could not be made concerning the photometric variability ofthe 14 remaining stars.

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Observation and Astrometry data

Constellation:Camelopardalis
Right ascension:11h11m00.38s
Declination:+80°56'56.0"
Apparent magnitude:7.726
Distance:436.681 parsecs
Proper motion RA:-20.6
Proper motion Dec:-7.8
B-T magnitude:8.68
V-T magnitude:7.805

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 96589
TYCHO-2 2000TYC 4555-1135-1
USNO-A2.0USNO-A2 1650-01505851
HIPHIP 54640

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