Recombination Atomic Data for Ionized Nebulae
The recombination coefficient atomic data were generated for use in proEQUIB and pyEQUIB:
-
rc_collection.fits, effective recombination coefficients for C II (Davey et al. 2000), N II (Escalante and Victor 1990), O II (Storey 1994; Liu et al. 1995), and Ne II ions (Kisielius et al. 1998), including Branching ratios (Br) for O II and N II ions.
-
rc_SH95.fits, hydrogenic ions for Z=1 to 8, namely H I, He II, Li III, Be IV, B V, C VI, N VII, and O VIII ions from Storey and Hummer (1995).
-
rc_PPB91.fits, effective recombination coefficients for H, He, C, N, O, Ne ions from Pequignot, Petitjean and Boisson (1991).
-
rc_he_ii_PFSD12.fits, effective He I recombination coefficients from Porter et al (2012) and (2013).
-
rc_n_iii_FSL13.fits, effective N II recombination coefficients from Fang, Storey and Liu (2011) and (2013).
-
rc_o_iii_SSB17.fits, effective O II recombination coefficients of 8889 recombination lines for Cases A, B, and C from Storey, Sochi and Bastin (2017). (Use these commends to unpack: tar -xvf rc_o_iii_SSB17.fits.tar.gz)
-
rc_o_iii_SSB17_orl_case_b.fits, effective O II recombination coefficients of 2433 optical recombination lines for Case B (Wavelength: 3500-9000Å) from Storey, Sochi and Bastin (2017). (Use this commend to unpack: tar -xvf rc_o_iii_SSB17_orl_case_b.fits.tar.gz)