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Mira model photospheres
Published online by Cambridge University Press: 04 August 2017
Abstract
The temperature stratifications and the emitted fluxes of Mira model photospheres based upon the extended density distribution of a pulsation model differ substantially from those of conventional model photospheres based upon a hydrostatic density distribution. Hence, the interpretation of Mira spectra by means of hydrostatic models is inadequate, and the spectral characteristics of Miras may deviate significantly from those of non-Miras.
- Type
- Stellar Coronae: Chromospheres of Cool Stars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 385 - 386
- Copyright
- Copyright © Reidel 1987