SWS spectral classification of ordinary stars

Details SWS spectral classification of ordinary stars SWS spectral classification of ordinary stars

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..329h&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 329

Physics

1

Stars, Classification

Scientific paper

We present an overview of the spectroscopic characteristics of ordinary stars observed with SWS in the low-resolution mode (R~250-400), covering the full instrumental wavelength range 2.38-45.2 μm. Our sample contains stars that fill a grid with spectral types between B and M, and luminosity classes dwarf to supergiant. We have identified the spectral features (H lines and molecular bands) that are of interest for classification purposes, and analyzed the dependence of the relative intensity of these features on spectral type and luminosity class.

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