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Paper: Comparing the Observed Frequencies of Balloon 09010001 with Theoretical Modes of Oscillation
Volume: 392, Hot Subdwarf Stars and Related Objects
Page: 277
Authors: Oreiro, R.; Baran, A.; Pérez Hernández, F.; Ulla, A.; Pigulski, A.
Abstract: Balloon 090100001 has turned out to be one of the most interesting pulsating sdB stars. However, its interest compares with the difficulty for it to be modelled. We present some clues or strategies from which some information can be inferred based on a comparison between observed and theoretical frequencies alone. These strategies might be applied to other pulsating sdBs.
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