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Constraining the degree of the dominant mode in QQ Vir

We present early results of the application of a method which uses multicolor photometry and spectroscopy for \ell discrimination. This method has been successfully applied to the pulsating hot subdwarf Balloon 090100001. Here we apply the method to QQ Vir (PG1325+101). This star was observed spectroscopically and photometrically in 2008. Details on spectroscopy can be found in Telting et al. (2010) while photometry and preliminary results on \ell discrimination are provided here. The main aim of this work was to compare the value of the \ell parameter derived for the main mode in QQ Vir to previously published values derived by using different methods.

preprint2010arXivOpen access
Andrzej BaranJohn TeltingRoy OstensenMaciej WiniarskiMarek DrozdzDorota KozielMike ReedRaquel OreiroRoberto SilvottiMichal SiwakUli HeberPeter Papics
astro-ph.SR
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Andrzej BaranJohn TeltingRoy OstensenMaciej WiniarskiMarek DrozdzDorota KozielMike ReedRaquel OreiroRoberto SilvottiMichal SiwakUli HeberPeter Papics

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