Titanium sulphide in the spectra of stellar atmospheres

Details Titanium sulphide in the spectra of stellar atmospheres Titanium sulphide in the spectra of stellar atmospheres

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.258p..49j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 258, no. 3, p. 49P-51P.

Astronomy and Astrophysics

Astronomy

12

Mira Variables, Stellar Atmospheres, Stellar Spectra, Sulfides, Titanium Compounds, Astronomical Spectroscopy, Molecular Spectra, Spectrum Analysis

Scientific paper

Two new transitions in the IR region - E3Pi-X3D and A3Phi-X3Delta - are
identified on the basis of laboratory studies of the spectrum of TiS.
These two transitions account for the IR absorptions between 1.15 and
1.35 micron observed by Hinkle et al. (1989) in R And and Chi Cyg. It is
concluded that these two stars cannot be regarded as pure type S stars.

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