Photometric detection of pulsations in the stars of the wide binary WDS 12483-6708

Details Photometric detection of pulsations in the stars of the wide binary WDS 12483-6708 Photometric detection of pulsations in the stars of the wide binary WDS 12483-6708

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.153...17s&link_type=abstract

Communications in Asteroseismology, Vol.153, p. 17-19

Computer Science

Scientific paper

We detected stellar pulsations in at least one of the components of the
wide double star WDS 12483-6708. The largest observed photometric
amplitude, in Stroemgren filter y, is around 0.02 magnitudes with period
about 0.02 days. The detection was based on five hours of differential
CCD photometry of the two double star components.

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