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On the formation of continuous spectrum and emission line profiles of P Cygni

Published online by Cambridge University Press:  14 August 2015

T. Nugis ,
I. Kolka  and
L. Luud
T. Nugis
Affiliation:
Tartu Astrophysical Observatory, Tôravere 202444 Estonia U.S.S.R.
I. Kolka
Affiliation:
Tartu Astrophysical Observatory, Tôravere 202444 Estonia U.S.S.R.
L. Luud
Affiliation:
Tartu Astrophysical Observatory, Tôravere 202444 Estonia U.S.S.R.

Extract

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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 

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