Abstract
Five more oscillating white dwarf stars have been discovered. The data now available from these and other sources support an explanation of observed oscillations in dwarf novae in terms of g-mode pulsations.
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WARNER, B., ROBINSON, E. Non-Radial Pulsations in White Dwarf Stars. Nature Physical Science 239, 2–7 (1972). https://doi.org/10.1038/physci239002a0
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DOI: https://doi.org/10.1038/physci239002a0
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