IRAS additional observations of classical novae

Abstract
Additional (pointed) observations of classical novae, obtained with the Infrared Astronomy Satellite (IRAS), are presented. The data include both old novae and novae in eruption. In the latter case, the IRAS data complement and confirm the results of ground-based infrared observations; while in the former case the IRAS data provide useful constraints on the long-term evolution of the material ejected in nova eruptions.

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