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À propos de : KPD 0629-0016, a slowly pulsating hot subdwarf star        

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  • KPD 0629-0016, a slowly pulsating hot subdwarf star
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  • The results of nine CCD photometric observing runs on KPD 0629-0016 are presented. During six of the runs measurements were obtained alternately through B and V filters. Four periodicities, for which there is good agreement between the frequencies identified in the B and V data, were extracted: these lie in the range 46-81 min. A fifth lower frequency appears to be definitely present, but is very uncertain due to aliasing. The ratios of the mode amplitudes measured in B and V, and the phase differences between variations in the two colours, are compatible with pulsation theory.
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