The Disruption of Molecular Cloud Cores by Photoionization
We solve the line transfer problem in evolving H ii regions in order to calculate line profiles of hydrogen recombination (Hα) and forbidden oxygen ([O III] 5007) lines along several lines of sight during the photo- disruption of molecular cloud cores, or high-density condensation. The density, velocity, and ionization structure of spherically
Franco, J. et al.
Fecha de publicación:
9
1995