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

Warning

This publication doesn't include Faculty of Arts. It includes Faculty of Science. Official publication website can be found on muni.cz.

Authors	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
Citation
web	http://www.aspbooks.org/a/volumes/table_of_contents/?book_id=590
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.
Related projects:	Velká infrastruktura CESNET Atmosféry a okolohvězdné prostředí magnetických horkých hvězd