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The Photometric Variability of Sun-like Stars: Observations and Results, 1984--1995
Using differential Stromgren b, y photometry, we monitored thebrightness variations of 41 program stars and their 73 comparison starsfrom 1984 through 1995. The predominantly main-sequence program starsspanned ranges of temperature and mean chromospheric activity centeredon solar values. About 40% of all the stars showed measurablevariability, typically at levels below 0.01 mag (~1%), on bothnight-to-night and year-to-year timescales. The variability correlatedwith mean chromospheric activity and advancing spectral type. We presentdifferential light curves and statistical descriptions of ourobservations.
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Observation and Astrometry data
| Constellation: | Αετός |
| Right ascension: | 20h05m10.88s |
| Declination: | +03°25'51.4" |
| Apparent magnitude: | 7.603 |
| Proper motion RA: | 0.6 |
| Proper motion Dec: | 4.6 |
| B-T magnitude: | 9.08 |
| V-T magnitude: | 7.725 |
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