3D hydrodynamic simulations of massive main-sequence stars -- IV. Internal gravity waves matter for SLF variability

Ähnliche Einträge

• 3D hydrodynamic simulations of massive main-sequence stars II. Convective excitation and spectra of internal gravity waves
  von: Thompson, William, et al.
  Veröffentlicht: (2023)
• 3D hydrodynamic simulations of massive main-sequence stars. III. The effect of radiation pressure and diffusion leading to a 1D equilibrium model
  von: Mao, Huaqing, et al.
  Veröffentlicht: (2023)
• Quantifying systematic uncertainties in white dwarf cooling age determinations
  von: Pathak, Praneet, et al.
  Veröffentlicht: (2024)
• Enhanced extra mixing in low-mass stars approaching the RGB tip and the problem of Li-rich red-clump stars
  von: Denissenkov, Pavel A., et al.
  Veröffentlicht: (2023)
• Photometric detection of internal gravity waves in upper main-sequence stars. IV. Comparable stochastic low-frequency variability in SMC, LMC, and Galactic massive stars
  von: Bowman, Dominic M., et al.
  Veröffentlicht: (2024)