Comparing the Observed Frequencies of Balloon 09010001 with Theoretical Modes of Oscillation

Bibcode
2008ASPC..392..277O
Oreiro, R.; Baran, A.; Pérez Hernández, F.; Ulla, A.; Pigulski, A.
Referencia bibliográfica

Hot Subdwarf Stars and Related Objects ASP Conference Series, Vol. 392, Proceedings of the conference held 23-27 July, 2007, at Otto-Friedrich-Universität, Bamberg, Germany. Edited by Ulrich Heber, C. Simon Jeffery, and Ralf Napiwotzki., p.277

Fecha de publicación:
0
2008
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro

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