An atlas of low-resolution near-infrared spectra of normal stars
Publications of the Astronomical Society of the Pacific1993Vol. 105, pp. 693–693
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Abstract
We present spectra of O to M stars, luminosity classes V, III, and Ib in the wavelength range 5800-8900 A, at approxiamtely 15 A resolution. We give identifications of the main spectral features and show that the stars follow well defined morphological sequences in both temperature and luminosity. This wavelength region and resolution, combined with the high sensitivity of silicon-based detectors, are very useful for spectral classification.
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