Classification of Stellar Spectra

M.M. Dworetsky
1990 International Astronomical Union Colloquium  
SummaryThe objectives of this exercise are to gain familiarity with the appearance of the spectra of stars, to understand some of the temperature and luminosity criteria used to classify spectra, and to gain insights into the relationship between the appearance of stellar spectra and physical conditions in stellar atmospheres.
doi:10.1017/s0252921100086565 fatcat:wtvg5imakvanvkojwikiwxijiq