This is the main table hosting the inputs and outputs of the models. In the 3MdB_17 database, it is named tab_17. Both tables are very similar, nevertheless some fields are only present in the tab_17, see below.
This table contains all the input parameters of the model and some of the outputs. The fields of the table ”tab” are described in the table below. In addition, the table contains the abundances (in log(X/H)) of the following elements: HYDROGEN , HELIUM , LITHIUM , BERYLLIUM , BORON , CARBON , NITROGEN , OXYGEN , FLUORINE , NEON , SODIUM , MAGNESIUM , ALUMINIUM , SILICON , PHOSPHORUS , SULPHUR , CHLORINE , ARGON , POTASSIUM , CALCIUM , SCANDIUM , TITANIUM , VANADIUM , CHROMIUM , MANGANESE , IRON , COBALT , NICKEL , COPPER , ZINC.
Line intensities are also part of the ”tab” table. All the lines are given in the Table of the page "lines". Notice that for every line, the field name (e. g. ”O__3_500684A”) refers to the volume integral of the line emissivity, while the field name ending with rad (e. g. ”O__3_500684A_rad”) refers to the line emissivity integrated over the radius. The intensities are given in erg/s. The 3MdB table contains 508 rows, the tab_17 version contains 762 rows.
New in 3MdB_17:
get_interp_cont(unit='WmHz', x_unit='GHz', x_value=2.5) from pyCloudy. The nebulae are at distance of 1kpc. Notice that the value obtained by this command does NOT take into account any cut in the nebula, the value is the one obtained for the complete model.