pith. sign in

arxiv: astro-ph/0209535 · v1 · submitted 2002-09-25 · 🌌 astro-ph

Model Photospheres with Accelerated Lambda Iteration

classification 🌌 astro-ph
keywords acceleratediterationlambdanon-lteproblemsolutionstatisticaladdress
0
0 comments X
read the original abstract

We address the classical stellar-atmosphere problem and describe our method of numerical solution in detail. The problem consists of the solution of the radiation transfer equation under the constraints of hydrostatic, radiative and statistical equilibrium (non-LTE). We employ the Accelerated Lambda Iteration (ALI) technique, and use statistical methods to construct non-LTE metal-line-blanketed model-atmospheres.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A systematic survey for hypervelocity runaways from thermonuclear supernovae

    astro-ph.SR 2026-06 unverdicted novelty 7.0

    A systematic survey with complete spectroscopic classification finds 13 hypervelocity D6 and LP 40-365 stars and shows that intermediate-heating evolutionary models best reproduce the observed population at birth rate...

  2. The origin of WHAM Point Source~46

    astro-ph.GA 2026-06 unverdicted novelty 4.0

    New spectroscopy rules out PG 0931+691 as ionizer of WPS 46 and associates the source with an IVC ionized by shocks.

  3. Studying hot evolved stars with ultraviolet spectroscopy

    astro-ph.IM 2026-06 unverdicted novelty 2.0

    Review of UV spectroscopy applications to hot evolved stars, emphasizing HST contributions and the need for continued observations ahead of HWO.