Briquet, M. ; Hubrig, S. ; De Cat, P. ; Aerts, C. ; North, P. ; Schöller, M.

published in Communications in Asteroseismology, 150, pp. 187 (2007)

Abstract: We carry out a comparative study between a sample of confirmed and well-studied B-type pulsators and a sample of well-studied Bp stars with known periods and magnetic field strengths. Our study indicates that the group of Bp stars is younger than the group of SPB stars and that stars with stronger magnetic fields have much lower pulsation amplitudes.

DOI: 10.1553/cia150s187
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