RACE-OC project: YSOs within 100pc (Messina+, 2010)

Details RACE-OC project: YSOs within 100pc (Messina+, 2010) RACE-OC project: YSOs within 100pc (Messina+, 2010)

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35209015m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/520/A15. Originally published in: 2010A&A...520A..15M

Physics

Clusters: Open, Stars: Late-Type, Stars: Variable

Scientific paper

Rotational periods of stars exhibiting rotational modulation due to photospheric magnetic activity (i.e., starspots) were determined by applying the Lomb-Scargle periodogram technique to photometric time-series data obtained by the All Sky Automated Survey (ASAS). The magnetic activity level was derived from the amplitude of the V lightcurves. The statistical significance of the rotational evolution at different ages was inferred by applying a two-sided Kolmogorov-Smirnov test to subsequent age-bins.
(3 data files).

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