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Search for Evidence of Radiative Equilibrium Departures in Extended Atmospheres
Published online by Cambridge University Press: 12 April 2016
Abstract
Through the analysis of line profiles of atoms in different ionization stages, we study the source function behavior of those elements that allow us to outline temperature structures in moving extended atmospheres. The radiative transfer equation is solved in the comoving frame and NLTE for multilevel atoms.
- Type
- 6. Disks
- Information
- International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 607 - 610
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
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