Modeling of multicomponent radiatively driven stellar winds using a Newton-Raphson method

Simple item page
dc.creatorKrticka, J.
dc.date2003-03-03
dc.date.accessioned2026-07-07T02:07:46Z
dc.date.available2026-07-07T02:07:46Z
dc.descriptionWe 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.
dc.description4 pages, to appear in Stellar Atmosphere Modeling, I. Hubeny, D. Mihalas, K. Werner eds., (San Francisco: ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0303030
dc.identifierhttp://arxiv.org/abs/astro-ph/0303030
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5804
dc.subjectAstrophysics
dc.titleModeling of multicomponent radiatively driven stellar winds using a Newton-Raphson method
dc.typetext

Files

Collections

arXiv