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We investigate the internal rotation profile of the GW Vir (PG1159-type) starPG 0122+200 by employing an asteroseismological model that closely reproducesthe observed periods of this star. We adopt a forward approach and twoinversion methods based on the rotational splitting of the pulsationfrequencies to explore the properties of the rotation of PG 0122+200. We foundevidence for differential rotation in this star.

The internal rotation of the GW Vir star PG 0112+200 through the eyes of asteroseismology