J. Van Beeck
Katholieke Universiteit Leuven
6 Papers
70 Citations
J. Van Beeck is an academic researcher from Katholieke Universiteit Leuven. The author has contributed to research in topics: Magnetic field & Rotation. The author has an hindex of 3, co-authored 6 publications.
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Papers
Period spacings of gravity modes in rapidly rotating magnetic stars
Vincent Prat,Stéphane Mathis,B. Buysschaert,J. Van Beeck,Dominic M. Bowman,Conny Aerts,C. Neiner +6 more
- 01 Jul 2019
TL;DR: In this article, the effect of an axisymmetric internal magnetic field on the frequency of gravity modes in rapidly rotating stars was studied and it was shown that a magnetic field with a near-core strength of the order of 150 kG leads to signatures that are detectable in period spacings for high-radial-order gravity modes.
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Detecting axisymmetric magnetic fields using gravity modes in intermediate-mass stars
J. Van Beeck,Vincent Prat,T. Van Reeth,Stéphane Mathis,Dominic M. Bowman,Coralie Neiner,Conny Aerts,Conny Aerts,Conny Aerts +8 more
TL;DR: In this paper, the influence of intrinsic magnetic fields on the magnitude of dipolar gravity mode frequency shifts in main-sequence stars with masses of 1.3, 2.0, and 3.0 was investigated.
Period spacings of gravity modes in rapidly rotating magnetic stars - I. Axisymmetric fossil field with poloidal and toroidal components
Vincent Prat,Stéphane Mathis,B. Buysschaert,B. Buysschaert,J. Van Beeck,Dominic M. Bowman,Conny Aerts,Conny Aerts,Coralie Neiner +8 more
TL;DR: In this article, the effect of an axisymmetric internal magnetic field on the frequency of gravity modes in rapidly rotating stars was studied and it was shown that a magnetic field with a near core strength of the order of 150 kG leads to signatures that are detectable in period spacings for high-radial-order gravity modes.
Period spacings of gravity modes in rapidly rotating magnetic stars - II. The case of an oblique dipolar fossil magnetic field
Vincent Prat,S. Mathis,S. Mathis,Coralie Neiner,J. Van Beeck,Dominic M. Bowman,Conny Aerts,Conny Aerts,Conny Aerts +8 more
TL;DR: In this paper, the effect of the obliquity of a mixed (poloidal and toroidal) dipolar internal fossil magnetic field with respect to the rotation axis on the frequency of gravity modes in rapidly rotating stars was investigated.
Period spacings of gravity modes in rapidly rotating magnetic stars I. Axisymmetric fossil field with poloidal and toroidal components
Vincent Prat,Stéphane Mathis,B. Buysschaert,B. Buysschaert,J. Van Beeck,Dominic M. Bowman,Conny Aerts,Conny Aerts,Coralie Neiner +8 more
TL;DR: In this paper, the effect of an axisymmetric internal magnetic field on the frequency of gravity modes in rapidly rotating stars was studied and it was shown that a magnetic field with a near-core strength of order 150 kG leads to signatures that are detectable in period spacings for high-radial-order gravity modes.