31 citations · 54 across the 2 of their papers we have counts for
3 papers
astro-ph.SR2021★ 23 cited
Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
T. Steindl, K. Zwintz, T. G. Barnes +2
Context: The pre-main sequence evolution is often simplified by choosing classical initial models. These have large initial radii and sufficient uniform contraction to make them fu…
astro-ph.SR2020
beta Cas: the first delta Scuti star with a dynamo magnetic field
K. Zwintz, C. Neiner, O. Kochukhov +10
F type stars are characterised by several physical processes such as different pulsation mechanisms, rotation, convection, diffusion, and magnetic fields. The rapidly rotating delt…
astro-ph.SR2019★ 31 cited
Revisiting the pulsational characteristics of the exoplanet host star Pictoris
K. Zwintz, D. R. Reese, C. Neiner +22
Exoplanet properties crucially depend on their host stars' parameters. In case the exoplanet host star shows pulsations, asteroseismology can be used for an improved description of…