Corpus ID: 115560408

ST Chamaeleontis and BP Coronae Australis: Two Southern Dwarf Novae Confirmed as Z Cam Stars

@article{Simonsen2014STCA,
  title={ST Chamaeleontis and BP Coronae Australis: Two Southern Dwarf Novae Confirmed as Z Cam Stars},
  author={M. Simonsen and T. Bohlsen and F. Hambsch and R. Stubbings},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2014}
}
  • M. Simonsen, T. Bohlsen, +1 author R. Stubbings
  • Published 2014
  • Physics
  • arXiv: Solar and Stellar Astrophysics
  • Z Camelopardalis (Z Cam) stars are a subset of dwarf novae distinguished by the occurrence of standstills, periods of relative constant brightness one to one and a half magnitudes fainter than maximum brightness. As part of an ongoing observing campaign, the Z CamPaign, the authors focused attention on several Z Cam suspects in the southern hemisphere. Two stars, BP Coronae Australis and ST Chamaeleontis were found to exhibit standstill behavior in 2013, thus confirming them as Z Cam type… CONTINUE READING
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