Modelling $δ$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution

Documents similaires

• Characterizing bright $δ$ Scuti pulsators using TESS lightcurves
  par: Mani, Prasad, et autres
  Publié: (2025)
• The $δ$ Scuti stars of the Cep--Her Complex. I: Pulsator fraction, rotation, asteroseismic large spacings, and the $ν_{\rm max}$ relation
  par: Murphy, Simon J., et autres
  Publié: (2024)
• The impact of radiative levitation on mode excitation of main-sequence B-type pulsators
  par: Rehm, R., et autres
  Publié: (2024)
• Chemically peculiar stars on the pre-main sequence
  par: Kueß, L., et autres
  Publié: (2024)
• The impact of disk-locking on convective turnover times of low-mass pre-main sequence and main sequence stars
  par: Landin, N. R., et autres
  Publié: (2024)