Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F03%3A00008047" target="_blank" >RIV/00216224:14310/03:00008047 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method

Original language description

We present a simple method for the solution of one-component and multicomponent hydrodynamic equations based on the Newton-Raphson method. We show that this method can be used for the solution of stationary hydrodynamic equations. This method has been used for the calculation of the low density stellar wind models for which the multicomponent nature of the wind influences the overall wind structure.

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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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)

Publication year

2003

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Stellar Atmosphere Modeling

ISBN

1-58381-131-1

ISSN

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e-ISSN

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Number of pages

4

Pages from-to

259-262

Publisher name

The Astronomical Society of the Pacific

Place of publication

San Francisco, USA

Event location

Tuebingen, Německo

Event date

Jan 1, 2002

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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