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

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rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
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. 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. (en) 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. (cs)
Title	Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method (en) Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method (cs)
skos:prefLabel	Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method (en) Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method (cs)
skos:notation	RIV/00216224:14310/03:00008047!RIV08-GA0-14310___
http://linked.open.../vavai/riv/strany	259-262
http://linked.open...avai/riv/aktivita	P
http://linked.open...avai/riv/aktivity	P(GA205/01/0656), P(GA205/02/0445)
http://linked.open...vai/riv/dodaniDat	2008
http://linked.open...aciTvurceVysledku	Krtička, Jiří
http://linked.open.../riv/druhVysledku	D - Článek ve sborníku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Masarykova univerzita / Přírodovědecká fakulta
http://linked.open...dnocenehoVysledku	615848
http://linked.open...ai/riv/idVysledku	RIV/00216224:14310/03:00008047
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	stars: mass-loss; stars: early-type; hydrodynamics (en)
http://linked.open.../riv/klicoveSlovo	stars: early-type stars: mass-loss hydrodynamics
http://linked.open...ontrolniKodProRIV	[AF4768A87E4B]
http://linked.open...v/mistoKonaniAkce	Tuebingen, Německo
http://linked.open...i/riv/mistoVydani	San Francisco, USA
http://linked.open...i/riv/nazevZdroje	Stellar Atmosphere Modeling
http://linked.open...in/vavai/riv/obor	BN
http://linked.open...ichTvurcuVysledku	1 (xsd:int)
http://linked.open...cetTvurcuVysledku	1 (xsd:int)
http://linked.open...vavai/riv/projekt	modeling of the extended envelopes of hot stars Physics of hot stars and stellar systems with hot components
http://linked.open...UplatneniVysledku	2003
http://linked.open...iv/tvurceVysledku	Krtička, Jiří
http://linked.open...vavai/riv/typAkce	WRD - Světová
http://linked.open.../riv/zahajeniAkce	2002-01-01 (xsd:date)
number of pages	4 (xsd:int)
http://purl.org/ne...btex#hasPublisher	The Astronomical Society of the Pacific
https://schema.org/isbn	1-58381-131-1
http://localhost/t...ganizacniJednotka	14310

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