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The ionization and thermal balance in P Cygni’s wind revisited
Published online by Cambridge University Press: 12 April 2016
Abstract.
The statistical and thermal equilibrium of P Cygni’s wind as a function of radius is investigated using the model of Drew (1985) with an improved treatment of hydrogen. Provisional calculated hydrogen and helium line fluxes are compared with observation. The wind temperature is found to be cooler than observation implies, and a further heating source is tentatively identified.
- Type
- Section II: Poster Papers, A Brief List of Catalogs, and Index
- Information
- International Astronomical Union Colloquium , Volume 113: Physics of Luminous Blue Variables , 1989 , pp. 263 - 264
- Copyright
- Copyright © Kluwer 1989