activity
20162020
most citedThree-Dimensional Simulations of Massive Stars: I. Wave Generation and Propagation

103 citations · 441 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR202035 cited

Recipes for bolometric corrections and Gaia luminosities of B-type stars: Application to an asteroseismic sample

May G. Pedersen, Ana Escorza, Peter I. Papics +1

We provide three statistical model prescriptions for the bolometric corrections appropriate for B-type stars as a function of: 1) T_eff, 2) T_eff, log g, and 3) T_eff, log g, [M/H]…

astro-ph.SR201931 cited

Isochrone-cloud fitting of the extended Main-Sequence Turn-Off of young clusters

C. Johnston, C. Aerts, M. G. Pedersen +1

Extended main-sequence turn-offs (eMSTO) are a commonly observed property of young clusters. A global theoretical interpretation for the eMSTOs is still lacking, but stellar rotati…

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…

astro-ph.SR201930 cited

Asteroseismology of massive stars with the TESS mission: the runaway Beta Cep pulsator PHL 346 = HN Aqr

Gerald Handler, Andrzej Pigulski, Jadwiga Daszyńska-Daszkiewicz +21

We report an analysis of the first known Beta Cep pulsator observed by the TESS mission, the runaway star PHL 346 = HN Aqr. The star, previously known as a singly-periodic pulsator…

astro-ph.SR201997 cited

Asteroseismic masses, ages, and core properties of Doradus stars using gravito-inertial dipole modes and spectroscopy

Joey S. G. Mombarg, Timothy Van Reeth, May G. Pedersen +5

The asteroseismic modelling of period spacing patterns from gravito-inertial modes in stars with a convective core is a high-dimensional problem. We utilise the measured period spa…