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IR Energy Distribution of OH/IR Sources

Published online by Cambridge University Press:  12 April 2016

W. A. Sherwood ,
E. Kreysa  and
G. V. Schultz
W. A. Sherwood
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 5300 Bonn, Federal Republic of Germany
E. Kreysa
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 5300 Bonn, Federal Republic of Germany
G. V. Schultz
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 5300 Bonn, Federal Republic of Germany

Extract

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Some infrared counterparts of Type II OHAR sources have been observed between 1µ and 30µ. In spite of their having very similar OH emission spectra, their energy distributions differ considerably among themselves from “flat” (1. 25µ to 4. 9µ) to “steep” (2. 2µ to 20µ). The energy distributions are compared with more familiar objects.

Type
Part III: Evolved Stars
Information
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 434 - 437
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

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