An atlas of low-resolution near-infrared spectra of normal stars

Details An atlas of low-resolution near-infrared spectra of normal stars An atlas of low-resolution near-infrared spectra of normal stars

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..693t&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 689, p. 693-720.

Mathematics

Logic

71

K Stars, M Stars, Near Infrared Radiation, O Stars, Stellar Spectra, Stellar Luminosity, Stellar Spectrophotometry, Stellar Temperature

Scientific paper

We present spectra of O to M stars, luminosity classes V, III, and Ib in the wavelength range 5800-8900 A, at approximately 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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