The Stellar Atmosphere Physical System II. An Operative Sequential Algorithm to Solve the Stellar Atmosphere Problem

Bibcode
2019SerAJ.198....1C
DOI
10.2298/SAJ190215001C
Crivellari, L.
Referencia bibliográfica

Serbian Astronomical Journal, vol. 198, pp. 1-11

Fecha de publicación:
6
2019
Número de autores
1
Número de autores del IAC
1
Número de citas
1
Número de citas referidas
1
Descripción
In this paper, the second and the last of the series, we present a sequential algorithm to solve the stellar atmosphere problem that may serve as a paradigm for the solution of more general non-linear and non-local problems. The Iteration Factors (IF) Method is applied to achieve a solution of the radiative transfer equations, consistent with the radiative equilibrium constraint.
Proyectos relacionados
Physical properties and evolution of massive stars
Propiedades Físicas y Evolución de Estrellas Masivas
Las estrellas masivas son objetos claves para la Astrofísica. Estas estrellas nacen con más de 8 masas solares, lo que las condena a morir como Supernovas. Durante su rápida evolución liberan, a través de fuertes vientos estelares, gran cantidad de material procesado en su núcleo y, en determinadas fases evolutivas, emiten gran cantidad de
Sergio
Simón Díaz
En ejecución
Tipo
Con árbitro
Métodos
Transferencia radiativa
Física estelar e interestelar (FEEI)
La Vía Láctea y el Grupo Local (MWLG)

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