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Table · dataset · 2013

Photometric rotation periods of stars in {alpha} Per

Listed in IVOA Registry (Virtual Observatory)

We present the results from a photometric monitoring program of primarily solar-type open cluster stars obtained during 1994 and 1995.

Description

Several members of the {alpha} Persei cluster have been monitored and the corresponding relation between coronal x-ray activity and rotation period derived. The relation among mid-G/K type members illustrates both the previously noticed downturn in L_X_/L_bol_ at high rotation rates and the sharp decrease in coronal activity at long rotation periods as seen among Pleiades stars.

Intensive observation of one slowly rotating G-type member of IC 4665 has enabled a period determination of 8-10 days to be made and illustrates the need for (and limitations of) high quality observations.

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