Pulsations and Period Changes of the SX Phoenicis Star DY Pegasi

Details Pulsations and Period Changes of the SX Phoenicis Star DY Pegasi Pulsations and Period Changes of the SX Phoenicis Star DY Pegasi

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009pasp..121..251f&link_type=abstract

Publications of the Astronomical Society of the Pacific, Volume 121, issue 877, pp.251-259

Astronomy and Astrophysics

Astronomy

3

Stars

Scientific paper

We present 83 new times of maximum light of the SX Phoenicis (SX Phe) star DY Pegasi (DY Peg), based mainly on our new time-series photometric observations from the years 2004-2008. Together with the times of maximum light in the literature, a comprehensive study of the 17.8 cd - 1 in the Fourier transformations of the new data sets, its signal-to-noise ratios were too low to detect this frequency.

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