Molecular absorption in the atmospheres of late-type giant stars

Details Molecular absorption in the atmospheres of late-type giant stars Molecular absorption in the atmospheres of late-type giant stars

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...92s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, May-June 1986, p. 92-94. In Russian.

Physics

Giant Stars, Late Stars, Molecular Absorption, Stellar Atmospheres, Atmospheric Attenuation, Spectral Bands, Zirconium Oxides

Scientific paper

The synthetic profile of the (0, 1) band of the B1Pi-X1Sigma(+) system of ZrO (693 nm) has been calculated using model atmospheres for S-type stars. The absorption of six bands of the gamma-system of ZrO was considered as a quasi-continuous one and was included in the continuous opacity. This procedure allows matching the observed band profile to the synthetic spectrum.

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