2009 20160701171657.0 10.1553/cia150s187 DOI ASTROimport-166 Briquet, M. 2007 A comparative study of B-type pulsators and non-pulsating chemically peculiar Bp stars 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. Hubrig, S. De Cat, P. Aerts, C. North, P. Schöller, M. Communications in Asteroseismology 150 2007 187 http://esoads.eso.org/abs/2007CoAst.150..187B published in REFERD