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Paper: The STELLA Open Cluster Survey – Rotational Evolution of Low-mass Stars: a Status Report
Volume: 448, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Page: 863
Authors: Fügner, D.; Granzer, T.; Strassmeier, K. G.
Abstract: Our study targets on measuring the rotational periods and absolute parameters of a well-selected sample of cool cluster stars. If an empirical law between rotational period, stellar age, and mass could be established it would provide valuable boundary conditions for evolutionary models. Current models predict a measurable difference of the rotational period between a solidly rotating and a differentially rotating star, and this could be tested. Our time-series observations are made in the Sloan r bandpass. Using image-stacking, we intend to boost the S/N to more than 500:1 even for the (early) M dwarfs in the fields. For calculations of stellar properties, like age, metallicity, gravity and surface temperature, we use the Strømgren system with few very deep exposures. In this paper, we present the survey outline, the instruments and the first steps already undertaken.
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