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.
Bibliographical reference

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

Advertised on:
0
2008
Number of authors
5
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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.
Type
Non-refereed

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