DQ Herculis: Synchronous Photometry

Details DQ Herculis: Synchronous Photometry DQ Herculis: Synchronous Photometry

Nov 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969sci...166..876n&link_type=abstract

Science, Volume 166, Issue 3907, pp. 876-877

Physics

Scientific paper

Synchronous signal averaging, applied to the photometry of the steller
system DQ Herculis in order to study the 71.1-second pulsations
discovered by Walker in 1956, yields a light curve which is a pure
sinusoid, within the accuracy of measurement. The binary period is
increasing, probably as a result of mass lost from the system.

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