The FUor Mass Distribution Matches the Solar Neighborhood IMF: Evidence for a Universal Eruptive Phase

Documenti analoghi

• Rosette Nebula Outburst Gaia 24djk from the Young Stellar Object V557 Mon
  di: Carvalho, Adolfo S., et al.
  Pubblicazione: (2025)
• Bolometric Corrections for FU Ori Object Accretion Disk Luminosities
  di: Carvalho, Adolfo S., et al.
  Pubblicazione: (2024)
• A Model for Eruptive Mass Loss in Massive Stars
  di: Cheng, Shelley J., et al.
  Pubblicazione: (2024)
• An Expanding Accretion Disk and a Warm Disk Wind As Seen In the Spectral Evolution of HBC 722
  di: Carvalho, Adolfo S., et al.
  Pubblicazione: (2024)
• The Present-Day Mass Function of Star Clusters in the Solar Neighborhood
  di: Pang, Xiaoying, et al.
  Pubblicazione: (2024)