Article: Reports outline astrophysics study findings from University of Vienna.

According to recent research published in the journal Astronomy & Astrophysics, "Asteroseismology has great potential for the study of metal-poor stars due to its sensitivity to determine stellar ages. Solid detections of oscillation frequencies in stars with well constrained fundamental parameters, combined with a known rotation period, should significantly advance our understanding of stellar structure and evolution in context with metallicity effects."

"Our goal was to detect p-mode oscillations in the metal-poor sub-dwarf 85 Peg A and to search for variability on longer timescales. We have obtained continuous high-precision optical photometry of the binary ...

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