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Photometric Variability in a Sample of 187 G and K Giants
We have used three automatic photoelectric telescopes to obtainphotometric observations of 187 G, K, and (a few) M0 field giants. Wefind low-amplitude photometric variability on timescales of days toweeks on both sides of the coronal dividing line (CDL) in a total of 81or 43% of the 187 giants. About one-third of the variables haveamplitudes greater than 0.01 mag in V. In our sample the percentage ofvariable giants is a minimum for late-G spectral classes and increasesfor earlier and later classes; all K5 and M0 giants are variable. Wealso obtained high-resolution, red wavelength spectroscopic observationsof 147 of the giants, which we used to determine spectralclassifications, vsini values, and radial velocities. We acquiredadditional high-resolution, blue wavelength spectra of 48 of the giants,which we used to determine chromospheric emission fluxes. We analyzedthe photometric and spectroscopic observations to identify the cause(s)of photometric variability in our sample of giants. We show that thelight variations in the vast majority of G and K giant variables cannotbe due to rotation. For giants on the cool side of the CDL, we find thatthe variability mechanism is radial pulsation. Thus, the variabilitymechanism operating in M giants extends into the K giants up to aboutspectral class K2. On the hot side of the CDL, the variability mechanismis most likely nonradial, g-mode pulsation.
| 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.
| Evidence for starspots on single solar-like stars
H-alpha intermediate-band and narrowband and lambda 4530 photoelectricphotometry carried out for five single main-sequence stars arepresented. For HD 149661, HD 152391, and HD 201091 low amplitudevariations of up to 0.04 mag at lambda 4530 are found. These variationsare attributable to the presence of starspots, and in the cases of HD149661 and HD 201091, an anti-correlation between the light variationand H-alpha and Ca II emission is found. Conclusions drawn from thisstudy include the idea that these three stars have active chromospheres,and that the light variation/Ca II and H-alpha variations are similar towhat is found in RS CVn systems.
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Observation and Astrometry data
| Constellation: | へびつかい座 |
| Right ascension: | 16h38m33.53s |
| Declination: | -01°13'53.5" |
| Apparent magnitude: | 6.723 |
| Distance: | 115.607 parsecs |
| Proper motion RA: | -14.7 |
| Proper motion Dec: | -11.4 |
| B-T magnitude: | 8.374 |
| V-T magnitude: | 6.86 |
Catalogs and designations:
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INHABITED SKY
