The brightness variability of active stars on different timescales by robotic observations

Details The brightness variability of active stars on different timescales by robotic observations The brightness variability of active stars on different timescales by robotic observations

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004an....325..660m&link_type=abstract

Astronomische Nachrichten, Vol.325, Issue 6, p.660-660

Astronomy and Astrophysics

Astronomy

6

Stars: Activity, Stars: Late-Type, Stars: Starspots, Stars: Rotation

Scientific paper

The brightness variations shown by late-type stars are caused by the presence and evolution of photospheric activity centers. In order to disentangle and correctly interpret the causes that contribute to the observed brightness variability on different time scales, late-type stars need to be observed systematically for several years e.g. by robotic telescopes.

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