Molecular structure in the envelopes of metal-rich red giants

Details Molecular structure in the envelopes of metal-rich red giants Molecular structure in the envelopes of metal-rich red giants

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983rbrfi..13..735r&link_type=abstract

Revista Brasileira de Fisica (ISSN 0374-4922), vol. 13, Dec. 1983, p. 735-746. Research supported by the Fundacao de Amparo a Pe

Computer Science

Abundance, Metallic Stars, Molecular Spectra, Red Giant Stars, Stellar Envelopes, Stellar Mass Ejection, Carbon, Hydrogen, Iron, Magnesium, Maser Outputs, Nitrogen, Oxygen, Silicon, Silicon Oxides, Sulfur

Scientific paper

Molecular and atomic abundances in metal-rich red giant envelopes are obtained, based on the dissociation equilibrium theory. A total of 53 molecular species composed of H, C, N, O, S, Si, Fe, and Mg is considered. For the SiO molecule, the column density is estimated along with some parameters relevant for the determination of the pumping mechanism responsible for the observed maser emission. The possibility of nucleation of some atomic and molecular species is also considered.

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