How the gradient of $M_{\rm d}$ versus UV field strength yields insights into the ages of protoplanetary disc populations

Documenti analoghi

• How the microphysical properties of external photoevaporation influence the global evolution of protoplanetary discs
  di: Coleman, Gavin A. L., et al.
  Pubblicazione: (2025)
• Magnetic disk winds in protoplanetary disks: Description of the model and impact on global disk evolution
  di: Kadam, Kundan, et al.
  Pubblicazione: (2025)
• Effects of stellar density on the photoevaporation of circumstellar discs
  di: Concha-Ramírez, Francisca, et al.
  Pubblicazione: (2020)
• The observable impact of runaway OB stars on protoplanetary discs
  di: Coleman, Gavin A. L., et al.
  Pubblicazione: (2025)
• The survivorship bias of protoplanetary disc populations
  di: Malanga, Lorenzo Alessio, et al.
  Pubblicazione: (2025)