Catastrophic Cooling in Superwinds. III. Non-equilibrium Photoionization
Supplementary Material
Table 1. Integrated luminosities (unit in erg/s) calculated by the NPI models (see Appendix A for machine-readable tables).
The compressed (tar.gz) file containing the machine-readable table files for the emission-line data (a portion shown for guidance regarding its form and content in Table 3) is available in the electronic edition of this article. The following machine-readable files for the emission-line data are available:
- table_NPI_radi.dat: Fully radiation-bounded non-equilibrium photoionization models.
- table_NPI_pden.dat: Partially density-bounded non-equilibrium photoionization models.
- table_NPI_dens.dat: Fully density-bounded non-equilibrium photoionization models.
Each file is named as table_case_bound.dat such as table_NPI_radi.dat, where case is for the ionization case (NPI: non-equilibrium photoionization), and bound for the optical depth model (radi: fully radiation-bounded, pden: partially density-bounded, and dens: fully density-bounded).
Each file contains the following information:
- metal: metallicity Ẑ ≡ Z/Z⊙ = 1, 0.5, 0.25, and 0.125.
- dMdt: mass-loss rate Ṁsc = 10−1, 10−2, 10−3, and 10−4 × Ẑ0.72 M⊙ yr−1.
- Vinf: wind terminal speed V∞ = 250, 500, and 1000 × Ẑ0.13 km s−1.
- Rsc: cluster radius Rsc = 1 pc.
- age: Cluster current age t = 1 Myr.
- Mstar: Cluster total stellar mass M★ = 2.05 × 106 M⊙.
- Lion: Logarithmic ionizing luminosity log Lion.
- Namb: ambient density namb = 1, 10, 102, and 103 cm−3.
- Tamb: mean ambient temperature Tamb determined by CLOUDY.
- Rmax: maximum radius Rmax (pc) for the surface brightness integration.
- Raper: aperture radius Raper (pc) for the total luminosity integration.
- Rshell: shell radius Rshell (pc).
- Rstr: Strömgren radius Rstr (pc) determined by CLOUDY.
- Rbin: bubble inner radius Rb,in (pc).
- Rbout: bubble outer radius Rb,out (pc) or shell inner radius.
- Tbubble: median temperature Tbubble of the hot bubble (region b in Figure 2).
- Tadi: median temperature Tadi,med of the expanding wind predicted by the adiabatic solutions (region a in Figure 2).
- Twind: median temperature Tw,med of the expanding wind predicted by MAIHEM with the radiative solutions (region a in Figure 2).
- logUsp: Logarithmic dimensionless ionization parameter log(Usph) in a spherical geometry calculated by CLOUDY, defined as Usph ≡ Q(H0)/4πR2strnHc, where Q(H0) is the total number of hydrogen-ionizing photons emitted per second, nH the hydrogen density, and c the speed of light.
- thin: optically thin (1) or thick (0) model.
- mode: the cooling/heating radiative/adiabatic modes:
- 1 (AW: adiabatic wind),
- 2 (AB: adiabatic bubble),
- 3 (AP: adiabatic, pressure-confined),
- 4 (CC: catastrophic cooling),
- 5 (CB: catastrophic cooling bubble), and
- 6 (CP: catastrophic cooling, pressure-confined).
- H_1_1216, H_1_6563, . . . , Ar_5_7006: integrated luminosities of the emission lines Lyα λ1216 Å, Hα λ6563 Å, . . . , [Ar V] λ7006 Å, respectively.