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New Infrared Results for Classical Novae

Published online by Cambridge University Press:  12 April 2016

Robert D. Gehrz
Robert D. Gehrz*
Affiliation:
Department of Astronomy, University of Minnesota,116 Church Street S.E., Minneapolis, MN 55455

Abstract

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Recent infrared studies of classical novae are described. The nucleation and growth of dust in nova ejecta was confirmed by optical/infrared photometry of several novae during the past five years including QU Vul, V842 Cen, V827 Her, and QV Vul. These novae provided evidence that dust of every astrophysical chemical and mineral composition can condense in nova ejecta. Infrared forbidden fine structure lines were identified in the recent novae V1819 Cyg, QU Vul, OS And, and V827 Her. The implication of IRAS measurements for nova energetics is discussed.

Type
1b. Novae During Outbursts
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 138 - 147
Copyright
Copyright © Springer-Verlag 1990

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