Dominic M. Bowman
Katholieke Universiteit Leuven
144 Papers
838 Citations
Dominic M. Bowman is an academic researcher from Katholieke Universiteit Leuven. The author has contributed to research in topics: Stars & Asteroseismology. The author has an hindex of 30, co-authored 117 publications. Previous affiliations of Dominic M. Bowman include Max Planck Society & University of Central Lancashire.
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Papers
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.
EPIC 201585823, a rare triple-mode RR Lyrae star discovered in K2 mission data
TL;DR: In this paper, a new triple-mode RR Lyr star, EPIC 201585823, was discovered in the Kepler K2 mission Campaign 1 data, which pulsates primarily in the fundamental and first-overtone radial modes, and a third non-radial mode.
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.
Detecting axisymmetric magnetic fields using gravity modes in intermediate-mass stars
Jordan Van Beeck,Vincent Prat,Timothy Van Reeth,Stéphane Mathis,Dominic M. Bowman,Coralie Neiner,Conny Aerts +6 more
TL;DR: In this paper, a fossil, axisymmetric internal magnetic field affects period spacing patterns of dipolar gravity mode oscillations in main-sequence stars with masses of 1.3, 2.0 and 3.0 M.
Asteroseismology of Massive Stars with the TESS Mission: The Runaway β Cep Pulsator PHL 346 = HN Aqr
Gerald Handler,Andrzej Pigulski,Jadwiga Daszyńska-Daszkiewicz,Andreas Irrgang,David Kilkenny,Zhao Guo,Norbert Przybilla,Filiz Kahraman Alicavus,Thomas Kallinger,J. Pascual-Granado,Ewa Niemczura,Tomasz Różański,S. Chowdhury,Derek Buzasi,G. M. Mirouh,Dominic M. Bowman,Cole Johnston,M. G. Pedersen,Sergio Simón-Díaz,Sergio Simón-Díaz,Ehsan Moravveji,Kosmas Gazeas,Peter De Cat,Roland Vanderspek,George R. Ricker +24 more
TL;DR: In this paper, the first known β Cep pulsator observed by the Transiting Exoplanet Survey Satellite (TESS) mission, the runaway star PHL 346 = HN Aqr, has at least 34 oscillation modes excited, 12 in the g-mode domain and 22 p modes.