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Article contents
On the formation of continuous spectrum and emission line profiles of P Cygni
Published online by Cambridge University Press: 14 August 2015
Extract
The attempts to interpret the values of the observed radio and infrared fluxes of P Cygni via simple mass outflow models (constant outflow velocity or usual radiative acceleration outflow) lead to a strong discrepancy between the observed and the calculated values.
- Type
- Session 1: Optical Spectroscopy
- Information
- Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 39 - 42
- Copyright
- Copyright © Reidel 1979