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Pulsation modes in B stars with variable line profiles
2008In this paper several observational characteristics of the line profile variable B stars (“53 Persei variables”) are discussed. These stars reside between 08 and B5 on the main sequence and extend perhaps to class I. We believe the 53 Per variables are a separate group related to the classical β Cephei variables.
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Determination of variability properties of candidate pulsating Am stars
The main goal of the study was to investigate the variability properties of candidate pulsating Am stars. Using TESS data and Eleanor software, light curves of 30 target stars were obtained. The light curves were fitted with a Fourier series to obtain Fourier transforms of the 30 target stars.Ssebaggala, Chrizestom +2 more
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The Pulsation Theory of Variable Stars
Physics Today, 1949Svein Rosseland, Lyman Spitzer
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Pulsating White Dwarf Stars and Precision Asteroseismology
Annual Review of Astronomy and Astrophysics, 2008Kepler, So
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Very regular high-frequency pulsation modes in young intermediate-mass stars
Nature, 2020Tim Bedding +2 more
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Outbursts of luminous blue variable stars from variations in the helium opacity
Nature, 2018Yan-Fei Jiang +2 more
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Angular momentum transport by heat-driven g-modes in slowly pulsating B stars
Monthly Notices of the Royal Astronomical Society, 2018Richard H D Townsend +1 more
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