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Full non-LTE spectral line formation III. The case of a two-level atom with broadened upper level

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dc.contributor.author Sampoorna, M
dc.contributor.author Paletou, F
dc.contributor.author Bommier, V
dc.contributor.author Lagache, T
dc.date.accessioned 2024-11-12T05:55:27Z
dc.date.available 2024-11-12T05:55:27Z
dc.date.issued 2024-10
dc.identifier.citation Astronomy & Astrophysics, Vol. 690, A213 en_US
dc.identifier.issn 0004-6361
dc.identifier.uri http://hdl.handle.net/2248/8574
dc.description Open Access en_US
dc.description Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
dc.description.abstract In the present paper we consider the full nonlocal thermodynamic equilibrium (non-LTE) radiation transfer problem. This formalism allows us to account for deviation from equilibrium distribution of both the radiation field and the massive particles. In the present study, two-level atoms with broadened upper level represent the massive particles. In the absence of velocity-changing collisions, we demonstrate the analytic equivalence of the full non-LTE source function with the corresponding standard non-LTE partial frequency redistribution (PFR) model. We present an iterative method based on operator splitting techniques that can be used to numerically solve the problem at hand. We benchmark it against the standard non-LTE transfer problem for a two-level atom with PFR. We illustrate the deviation of the velocity distribution function of excited atoms from the equilibrium distribution. We also discuss the dependence of the emission profile and the velocity distribution function on elastic collisions and velocity-changing collisions. en_US
dc.language.iso en en_US
dc.publisher EDP Sciences en_US
dc.relation.uri https://doi.org/10.1051/0004-6361/202449722
dc.rights © The Authors 2024
dc.subject Line: formation en_US
dc.subject Line: profiles en_US
dc.subject Radiation mechanisms: general en_US
dc.subject Radiative transfer en_US
dc.subject Methods: numerical en_US
dc.subject Stars: atmospheres en_US
dc.title Full non-LTE spectral line formation III. The case of a two-level atom with broadened upper level en_US
dc.type Article en_US


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