Bibcode
Crivellari, L.
Bibliographical reference
Serbian Astronomical Journal, vol. 198, pp. 1-11
Advertised on:
6
2019
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
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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