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3-D NLTE Monte Carlo radiative transfer code for stellar wind modeling

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FIŠÁK Jakub JIŘÍ Kubát BRANKICA Kubátová MARKUS Kromer JIŘÍ Krtička

Year of publication 2019
Type Article in Proceedings
Conference Radiative Signatures from the Cosmos
MU Faculty or unit

Faculty of Science

Keywords Monte Carlo; Radiative transfer; Stellar winds; Macroatom
Description We present the current state of our 3-D Monte Carlo radiative transfer code for modelling the stellar wind of hot stars. The code uses the concept of indivisible energy packets proposed by Leon Lucy. Currently the code calculates the emergent spectrum of an input stellar wind model. The code is being developed to solve the NLTE line formation problem in a 3-D model of a stellar wind.
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