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[ascl:2112.014] Qwind3: Modeling UV line-driven winds originating from accretion discs

Qwind3 models radiation-driven winds originating from accretion discs. An improvement over Qwind (ascl:2112.013), it derives the wind initial conditions and has significantly improved ray-tracing to calculate the wind absorption self consistently given the extended nature of the UV emission. It also corrects the radiation flux for relativistic effects, and assesses the impact of this on the wind velocity.

Code site:
https://github.com/arnauqb/Qwind.jl
Described in:
https://ui.adsabs.harvard.edu/abs/2021arXiv211102742Q
Bibcode:
2021ascl.soft12014Q

Views: 1567

ascl:2112.014
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