Results 271 to 275 of about 501 (275)
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Physical Basis of the Pulsation Theory of Variable Stars
Annual Review of Astronomy and Astrophysics, 1963A brief historical survey of the development of the pulsation theory of stellar variability is given. The problem of stellar auto-oscillations, the physical basis of the theory of stellar variability, and the universal interpretation of the different types of pulsating variable stars are discussed. (C.E.S.)
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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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