Contribution of the Electron Scattering Process to the Broad Hα Wings

We modeled the extended wings of the OVI 1032, 1038 Å resonance lines and He II 1640 Å emission line in the spectra of Z And, AG Dra and V1016 Cyg by the electron scattering process. By this way we determined the electron temperature and the electron optical depth of the layer of electrons, through...

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Bibliographic Details
Main Authors: Sekeráš M., Skopal A.
Format: Article
Language:English
Published: De Gruyter 2012-06-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2017-0378