• Corpus ID: 248496827

Negative superhumps in the eclipsing Z Cam + VY Scl star ES Dra

@inproceedings{Kato2022NegativeSI,
  title={Negative superhumps in the eclipsing Z Cam + VY Scl star ES Dra},
  author={Taichi Kato},
  year={2022}
}
I analyzed All-Sky Automated Survey for Supernovae (ASAS-SN) Sky Patrol data of ES Dra and clas-sified it to be a Z Cam star with VY Scl-type fading episodes. An analysis of Transiting Exoplanet Survey Satellite (TESS) observations showed that this object shows shallow eclipses and that the orbital period is 0.17749895(17) d. Negative superhumps with a period of 0.167830(2) d and the beat phenomenon between the period of negative superhumps and the orbital period were detected in the TESS data… 

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