The single-sided pulsator CO Camelopardalis

@article{Kurtz2020TheSP,
  title={The single-sided pulsator CO Camelopardalis},
  author={D. Kurtz and G. Handler and S. Rappaport and H. Saio and J. Fuller and T. Jacobs and A. Schmitt and D. Jones and A. Vanderburg and D. Lacourse and L. Nelson and F. Aliccavucs and M. Giarrusso},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2020},
  volume={494},
  pages={5118-5133}
}
  • D. Kurtz, G. Handler, +10 authors M. Giarrusso
  • Published 2020
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • Abstract CO Cam (TIC 160268882) is the second “single-sided pulsator” to be discovered. These are stars where one hemisphere pulsates with a significantly higher amplitude than the other side of the star. CO Cam is a binary star comprised of an Am δ Sct primary star with Teff = 7070 ± 150 K, and a spectroscopically undetected G main-sequence secondary star. The dominant pulsating side of the primary star is centred on the L1 point. We have modelled the spectral energy distribution combined with… CONTINUE READING
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