Ref: ASTROimport-166

A comparative study of B-type pulsators and non-pulsating chemically peculiar Bp stars

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
Links: link

The record appears in these collections:
Royal Observatory of Belgium > Astronomy & Astrophysics
Science Articles > Peer Reviewed Articles

 Record created 2016-07-01, last modified 2016-07-01