The classification and interpretation of S stars

Details The classification and interpretation of S stars The classification and interpretation of S stars

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phdt.........2p&link_type=abstract

Ph.D. Thesis Indiana Univ., Bloomington.

Astronomy and Astrophysics

Astrophysics

9

Late Stars, Mathematical Models, Near Infrared Radiation, Stellar Spectra, Stellar Spectrophotometry, Astrophysics, Data Reduction, Spectrum Analysis

Scientific paper

An 8-color near-infrared photometric system was used to sample the stellar flux of approximately 160 stars of many spectral types to provide a blackbody color temperature, an infrared magnitude (at 1.04 microns), and molecular band strength indices of TiO, VO, ZrO, CN, and an unidentified feature. Based upon this data, classification sub-groups were established with the color temperature and band strengths of TiO and ZrO and used to subdivide the S stars into homogenous groups with respect to their physical variables and to estimate the values of the variables of those sub-groups.

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