Peculiarities of the molecular abundances in the atmospheres of substars

Details Peculiarities of the molecular abundances in the atmospheres of substars Peculiarities of the molecular abundances in the atmospheres of substars

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17....3z&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 1, p. 3-16

Physics

2

Scientific paper

Equilibrium gas phase concentrations of molecular species are calculated within the LTE approximation in a H, He-based system (X = 0.70, Y = 0.27, Z = 0.03) with an addition of carbon, nitrogen, and oxygen, one percent by weight per element. In all 115 molecules, ions, and radicals are taken into account. The most abundant chemical species are determined for each elements. The ionic forms governing the charge balance in the system are also specified and discussed.

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