activity
20122020
most citedLow-frequency gravity waves in blue supergiants revealed by high-precision space photometry

165 citations · 583 across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.SR202036 cited

Two-Dimensional Simulations of Internal Gravity Waves in The Radiation Zones of Intermediate-Mass Stars

R. P. Ratnasingam, P. V. F. Edelmann, T. M. Rogers

Intermediate-mass main sequence stars have large radiative envelopes overlying convective cores. This configuration allows internal gravity waves (IGWs) generated at the convective…

astro-ph.SR2020103 cited

Photometric detection of internal gravity waves in upper main-sequence stars. II. Combined TESS photometry and high-resolution spectroscopy

D. M. Bowman, S. Burssens, S. Simón-Díaz +5

Context. Massive stars are predicted to excite internal gravity waves (IGWs) by turbulent core convection and from turbulent pressure fluctuations in their near-surface layers. The…

astro-ph.SR202061 cited

Fully compressible simulations of waves and core convection in main-sequence stars

L. Horst, P. V. F. Edelmann, R. Andrassy +4

Context. Recent, nonlinear simulations of wave generation and propagation in full-star models have been carried out in the anelastic approximation using spectral methods. Although…

astro-ph.SR2019165 cited

Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry

Dominic M. Bowman, Siemen Burssens, May G. Pedersen +14

Almost all massive stars explode as supernovae and form a black hole or neutron star. The remnant mass and the impact of the chemical yield on subsequent star formation and galacti…

astro-ph.SR2019103 cited

Three-Dimensional Simulations of Massive Stars: I. Wave Generation and Propagation

P. V. F. Edelmann, R. P. Ratnasingam, M. G. Pedersen +3

We present the first three-dimensional (3D), hydrodynamic simulations of the core convection zone (CZ) and extended radiative zone spanning from 1% to 90% of the stellar radius of…

astro-ph.SR2019

Astro2020 Science White Paper: gravity-wave asteroseismology of intermediate- and high-mass stars

Andrew Tkachenko, Conny Aerts, Dominic M. Bowman +17

The evolution of a star is driven by the physical processes in its interior making the theory of stellar structure and evolution the most crucial ingredient for not only stellar ev…