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Uy phoenicis: RR lyrae variable, not dwarf nova

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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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  1. Hoffmeister, C.: 1963,Veröffentl. Stern. Sonnenberg 6, No. 1.

  2. Ledoux, P. and Walraven, Th.: 1958,Hand. der Physik 51, 353.

  3. Meinunger, I.: 1973,Mitt. Veränd. Stern. 6, 87.

  4. Saha, A.: 1984,Astrophys. J. 283, 580.

  5. Saha, A.: 1985,Astrophys. J. 289, 310.

  6. Vogt, N. and Bateson, F. M.: 1982,Astron. Astrophys. Suppl. 48, 383.

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

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  • Spectroscopic Observation
  • Dwarf Nova