Note: unless otherwise stated, the broadening coefficients for the principal (most abundant) isotopologue can be used for other isotopologues of the same molecule.
- 12C3__O2.broad
C3 - O2 pressure broadening parameters (main isotopologue).
- 12C3__NO.broad
C3 - NO pressure broadening parameters (main isotopologue).
- 12C3__NH3.broad
C3 - NH3 pressure broadening parameters (main isotopologue).
- 12C3__N2.broad
C3 - N2 pressure broadening parameters (main isotopologue).
- 12C3__He.broad
C3 - He pressure broadening parameters (main isotopologue).
- 12C3__H2O.broad
C3 - H2O pressure broadening parameters (main isotopologue).
- 12C3__H2.broad
C3 - H2 pressure broadening parameters (main isotopologue).
- 12C3__CO2.broad
C3 - CO2 pressure broadening parameters (main isotopologue).
- 12C3__CO.broad
C3 - CO pressure broadening parameters (main isotopologue).
- 12C3__CH4.broad
C3 - CH4 pressure broadening parameters (main isotopologue).
- 12C3__Ar.broad
C3 - Ar pressure broadening parameters (main isotopologue).
- 12C3__self.broad
C3 - self pressure broadening parameters (main isotopologue).
References
- Buldyreva, J., Stehlin, K., Yurchenko, S.N., Guest, E.R., Tennyson, J., "Semiclassical Estimates of Pressure-induced Line Widths for Infrared Absorption in Hot (Exo)planetary Atmospheres", The Astrophysical Journal Supplement Series 276, 23 (2024). [link to article]