Monitoring solar-type stars

Physics

Scientific paper

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Dwarf Stars, Photometry, Solar Flux, Stellar Luminosity, Variable Stars, Variations, Measuring Instruments, Optical Measurement, Solar Physics, Stars, Theoretical Physics

Scientific paper

Old UBV and recent uvby photometry of solar-type dwarfs and other
standard stars yield an upper limit of variability (determined by
observational errors) of about 0.004 mag rms. A factor two improvement
in this upper limit is achievable.

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