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
The CubeSpec space mission: Asteroseismology of massive stars from time-series optical spectroscopy
Dominic M. Bowman,Bart Vandenbussche,Hugues Sana,A. Tkachenko,Gert Raskin,Tjorven Delabie,Brian VanDoren,Pierre Royer,S. Garcia,T. Van Reeth,the CubeSpec Collaboration +10 more
- 18 Jul 2022
TL;DR: The CubeSpec mission as discussed by the authors was designed to provide low-cost space-based high-resolution optical spectroscopy for pulsation mode identification from spectroscopic line and empower asteroseismology of massive stars.
Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry
Dominic M. Bowman,Siemen Burssens,M. G. Pedersen,Cole Johnston,Conny Aerts,Conny Aerts,B. Buysschaert,B. Buysschaert,Mathias Michielsen,Andrew Tkachenko,Tamara M. Rogers,Tamara M. Rogers,P. V. F. Edelmann,R. P. Ratnasingam,Sergio Simón-Díaz,Norberto Castro,Ehsan Moravveji,Benjamin J. S. Pope,Timothy R. White,Peter De Cat +19 more
TL;DR: The discovery of variability in blue supergiants is a step towards a data-driven empirical calibration of theoretical evolution models for the most massive stars in the Universe as mentioned in this paper, which will provide constraints on ages, core masses, interior mixing, rotation and angular momentum transport.
MOBSTER - IV. Detection of a new magnetic B-type star from follow-up spectropolarimetric observations of photometrically selected candidates★
A. David-Uraz,A. David-Uraz,A. David-Uraz,Matt Shultz,Véronique Petit,Dominic M. Bowman,C. Erba,R. Fine,Coralie Neiner,Herbert Pablo,J. Sikora,Asif ud-Doula,Gregg A. Wade +12 more
TL;DR: In this paper, the authors presented results from the spectropolarimetric follow-up of photometrically selected candidate magnetic B stars from the MOBSTER project, and reported the discovery of a previously unknown spectroscopic binary system, HD 25709.
Three-dimensional Simulations of Massive Stars. I. Wave Generation and Propagation
P. V. F. Edelmann,R. P. Ratnasingam,M. G. Pedersen,Dominic M. Bowman,Vincent Prat,Tamara M. Rogers,Tamara M. Rogers +6 more
TL;DR: In this paper, a 3D hydrodynamic simulation of the core convection zone (CZ) and extended radiative zone spanning from 1% to 90% of the stellar radius of an intermediate mass (3 $\mathrm{M}_\odot$) star is presented.
Combining WASP and Kepler data: the case of the δ Sct star KIC 7106205
TL;DR: In this article, ground-based photometric observations from Wide Angle Search for Planets (WASP) have been calibrated, scaled and combined with Kepler observations of the δ Sct star KIC 7106205, allowing them to extend the time base of the study of the unexplained amplitude and frequency variation of a single pressure mode at ν = 13.3942 d−1 by 2 yr.