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Short-period variability of the Be star ? Eri
Astrophysics and Space Science, 1984Photoelectric and spectrographic observations of the Be star λ Eri made during five nights indicate that the luminosity variations have a different periodicity from that of radial velocity variations. This result seems to show that, at least during our observing time, the observed variability has not to be ascribed to a pulsation of the star.
E. Antonello, L. Mantegazza, L. Pastori
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The Distribution of The Periods of the Hagnetic Variable Stars
International Astronomical Union Colloquium, 1976SummaryThe distribution of the periods of about 80 of the known variable Ap stars is studied in the framework of the oblique rotator model. It is shown that for the long period variables (P > 100 days) the oblique rotator has trouble in explaining the observed variations.
F.A. Catalano, G. Strazzulla
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Periodic variable A-F spectral type stars in the northern TESS continuous viewing zone
Astronomy and Astrophysics, 2022Jiří Liska +2 more
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Classification of periodic variable stars with novel cyclic-permutation invariant neural networks
Monthly Notices of the Royal Astronomical Society, 2021Joshua Bloom +2 more
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The Long-Period Variable Stars
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The ASAS-SN catalogue of variable stars – IV. Periodic variables in the APOGEE survey
Monthly Notices of the Royal Astronomical Society, 2019Thomas W -S Holoien +2 more
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