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Medium Resolution Spectroscopy at 1-2 Microns
Published online by Cambridge University Press: 12 April 2016
Abstract
The need for establishing classification criteria at long wavelengths is stressed. The usefulness of doing this is illustrated with a discussion of the composite spectra of FU Orionis stars. Spectra of these pre-main-sequence stars from 1.5-2.5μ were obtained with a Fourier Transform Spectrometer. Luminosity criteria in the l-2μ range are also discussed with application to M stars.
- Type
- V Classification related Spectrophotometry by Classical Techniques and by New Registration and Detection Methods
- Information
- International Astronomical Union Colloquium , Volume 47: Spectral Classification of the Future , 1979 , pp. 239 - 246
- Copyright
- Copyright © Vatican Observatory 1979