Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apjs...59...33p&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 59, Sept. 1985, p. 33-61.
Astronomy and Astrophysics
Astrophysics
95
Galaxies, Stellar Spectrophotometry, Electrophotometry, Metallicity, Spectral Line Width, Stellar Color, Stellar Spectra, Tables (Data)
Scientific paper
Continuous spectrophotometry has been obtained for 200 objects at a resolution of 10-17 A over the wavelength region 3600-10,000 A. Kron-Cousins BVRI colors are computed from the spectra and compared with published photoelectric photometry. The (V - R)C color index is used to group the individual observations to form synthesis standard spectra for 48 common spectral types. The standard groups include a solar abundance sequence of most spectral types and luminosity classes, metal-rich and metal weak G - K giant-branch sequences, and horizontal-branch giants. The variations with color, luminosity, and metallicity of several prominent line strengths are discussed. The spectral atlas is available as a FITS magnetic tape.
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