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The Infrared Spectrum of P Cygni

Published online by Cambridge University Press:  03 August 2017

J. R. Deacon  and
M. J. Barlow
J. R. Deacon
Affiliation:
Department of Physics & Astronomy University College London Gower Street, London WC1E 6BT
M. J. Barlow
Affiliation:
Department of Physics & Astronomy University College London Gower Street, London WC1E 6BT

Abstract

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An energy distribution for P Cyg (B1 Ia+) has been produced using UKIRT photometry and spectra, flux-calibrated IUE high-resolution spectra, Johnson and Mitchell 13-colour photometry and IRAS photometry. Infrared excesses due to free-free emission from the wind have then been derived and modelled.

Type
Session VII. Evolution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 558
Copyright
Copyright © Kluwer 1991