Project Details
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The age distribution of stars in the immediate solar environment

Subject Area Astrophysics and Astronomy
Term from 2015 to 2019
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 283666120
 
Final Report Year 2020

Final Report Abstract

The project goal, i.e., the determination of rotation periods of a complete sample of nearby stars, could not be fully reached. It is a little sobering to realize that a fundamental parameter of a star such as its rotation rate cannot be (easily) determined for even those stars that are most amenable to studies. In the end this is of course not surprising. If we were faced with a completely immaculate star without any surface inhomogeneities, we could determine only its v-sin(i) value, and for slow rotators this is next to impossible. Also the Sun, when viewed as a star, does not easily offer the luxury to measure its period through rotational modulation in integral light, one has to select the proper wavelength range and period. In the course of the project work we obtained quite a few new and unexpected results, some of the ”bread and butter” type (such as new binaries with their orbits) and other quite exciting results such as the discovery of short term magnetic cycles on the order of a few months for F-type stars.

Publications

 
 

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