RT06 Test #2 (Strömgren Sphere, thermal evolution allowed)¶
Test #2 from the Radiative Transfer Comparison Project (Iliev et al. 2006).
This problem investigates the growth of an HII region around a blackbody source of ionizing photons. The main parameters are:
Stellar ionizing photon production rate of \(\dot{Q} = 5 \times 10^{48} \ \text{s}^{-1}\).
Stellar spectrum is a \(10^5\) K blackbody.
Medium composed of hydrogen only, with a density of \(n_{\text{H}} = 10^{-3} \ \text{cm}^{-3}\).
Gas temperature is able to evolve. It is initially set to \(T=100\) K everywhere on the grid.
The ionization and heating rates are computed treating the source’s spectral energy distribution in full. A lengthy discussion of this can be found in Mirocha et al. (2012).
import ares
sim = ares.simulations.RaySegment(problem_type=2)
sim.run()
sim.PlotIonizationFrontEvolution(fig=1)
# Snapshots at 10 and 50 Myr
ax = sim.RadialProfile('h_1', fig=2, t=[10, 50])
sim.RadialProfile('h_2', ax=ax, t=[10, 50], ls='--')
sim.RadialProfile('Tk', fig=3, t=[10, 50])