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The Infrared Spectrum of P Cygni
Published online by Cambridge University Press: 03 August 2017
Abstract
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
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- Copyright © Kluwer 1991