Hostname: page-component-77c89778f8-vsgnj Total loading time: 0 Render date: 2024-07-20T22:37:00.397Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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