arXiv · 1108.3361
The internal rotation of the GW Vir star PG 0112+200 through the eyes of asteroseismology
Abstract
We investigate the internal rotation profile of the GW Vir (PG1159-type) star PG 0122+200 by employing an asteroseismological model that closely reproduces the observed periods of this star. We adopt a forward approach and two inversion methods based on the rotational splitting of the pulsation frequencies to explore the properties of the rotation of PG 0122+200. We found evidence for differential rotation in this star.
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A. H. Córsico, L. G. Althaus, S. D. Kawaler, M. M. Miller Bertolami, E. García-Berro. 2011-08-16. The internal rotation of the GW Vir star PG 0112+200 through the eyes of asteroseismology. https://arxiv.org/abs/1108.3361
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