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Uy phoenicis: RR lyrae variable, not dwarf nova

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Abstract

Photometric and spectroscopic observations of UY Phe, previously classified as a dwarf nova, show it to be a typea RR Lyr halo variable with a period of 0.5118 day.

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References

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Warner, B., Barrett, P. Uy phoenicis: RR lyrae variable, not dwarf nova. Astrophys Space Sci 124, 199–201 (1986). https://doi.org/10.1007/BF00649760

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Keywords

  • Spectroscopic Observation
  • Dwarf Nova