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