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Photographic Infrared Spectroscopy and Near Infrared Photometry of Be Stars: (Review Paper)

Published online by Cambridge University Press:  14 August 2015

J. P. Swings
J. P. Swings*
Affiliation:
Institut d'Astrophysique, B-4200 Cointe-Ougrée, Belgium

Extract

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As the title indicates two topics will be tackled in this presentation: spectroscopy and photometry. Let us therefore define first what ‘infrared’ means for these two subjects. I chose the following definitions:

  1. – photographic infrared spectroscopy: wavelengths Hα ≤ λ < 1.2 μ

  2. – near infrared photometry: wavebands: 1.6 μ ≤ λ ≤ 20 μ

Type
Part III: New Observational Techniques
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 219 - 225
Copyright
Copyright © Reidel 1976 

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