X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates

Documenti analoghi

• Habitable Zone and Atmosphere Retention Distance (HaZARD) Stellar-evolution-dependent loss models of secondary atmospheres
  di: Van Looveren, Gwenaël, et al.
  Pubblicazione: (2025)
• Long-term X-ray variability of the multiple-planet host L 98-59: Hints of an activity cycle
  di: Pillitteri, I., et al.
  Pubblicazione: (2025)
• Coping with loss: Stability of mass transfer from post-main sequence donor stars
  di: Temmink, K. D., et al.
  Pubblicazione: (2022)
• Impact of main-sequence mass loss on the appearance, structure and evolution of Wolf-Rayet stars
  di: Josiek, Joris, et al.
  Pubblicazione: (2024)
• Debris disks around main-sequence stars
  di: Pearce, Tim D.
  Pubblicazione: (2024)