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.
Bibliographical reference

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

Advertised on:
6
2019
Number of authors
1
IAC number of authors
1
Citations
1
Refereed citations
1
Description
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.
Related projects
Projets' image
Physical properties and evolution of Massive Stars
This project aims at the searching, observation and analysis of massive stars in nearby galaxies to provide a solid empirical ground to understand their physical properties as a function of those key parameters that gobern their evolution (i.e. mass, spin, metallicity, mass loss, and binary interaction). Massive stars are central objects to
Sergio
Simón Díaz
In progress
Type
Refereed
Methods
Radiative transfer
Stellar & Interstellar Physics (FEEI)
The Milky Way and the Local Group (MWLG)

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