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Model Photospheres with Accelerated Lambda Iteration

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arxiv astro-ph/0209535 v1 pith:AGDW7QFJ submitted 2002-09-25 astro-ph

classification astro-ph
keywords acceleratediterationlambdanon-lteproblemsolutionstatisticaladdress
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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.

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Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 21 citations worldwide. Full citation record

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    About 20% of 727 hot subdwarf stars observed by LAMOST show calcium absorption and reddening excesses that the authors attribute to long-lived circumstellar matter ejected during a common-envelope phase.

  4. The origin of WHAM Point Source~46

    astro-ph.GA 2026-06 unverdicted novelty 4.0 of 10

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

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

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