3-D NLTE Monte Carlo radiative transfer code for stellar wind modeling
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F19%3A00107799" target="_blank" >RIV/00216224:14310/19:00107799 - isvavai.cz</a>
Result on the web
<a href="http://www.aspbooks.org/a/volumes/table_of_contents/?book_id=590" target="_blank" >http://www.aspbooks.org/a/volumes/table_of_contents/?book_id=590</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
3-D NLTE Monte Carlo radiative transfer code for stellar wind modeling
Original language 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.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10300 - Physical sciences
Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Radiative Signatures from the Cosmos
ISBN
9781583819258
ISSN
1050-3390
e-ISSN
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Number of pages
6
Pages from-to
15-20
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Sorbonne University Paris
Event date
Jan 1, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000494866300003