Asteroseismology of the β Cephei star ν Eridani using differentially-rotating models

Details Asteroseismology of the β Cephei star ν Eridani using differentially-rotating models Asteroseismology of the β Cephei star ν Eridani using differentially-rotating models

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..211s&link_type=abstract

Communications in Astroseismology, Vol. 150, p.211

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This work is focused on asteroseismic modelling of B stars using differential rotation in both the equilibrium models and the oscillation computations. We discuss the possibility of inferring information on the internal structure from the analysis of asymmetries of rotationally split modes. In particular we present some preliminary results on the well-known β Cephei star ν Eridani for which at least three triplets have been identified as g_1, p_1 and p_2 (ℓ=1), respectively.

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