The classical stellar atmosphere problem

被引：93

作者：

Werner, K ^{[1
]}

Dreizler, S ^{[1
]}

机构：

[1] Univ Tubingen, Inst Astron & Astrophys, D-72076 Tubingen, Germany

来源：

JOURNAL OF COMPUTATIONAL AND APPLIED MATHEMATICS | 1999年 / 109卷 / 1-2期

关键词：

D O I：

10.1016/S0377-0427(99)00154-5

中图分类号：

O29 [应用数学];

学科分类号：

070104 ;

摘要：

We introduce the classical stellar atmosphere problem and describe in detail its numerical solution. The problem consists of the solution of the radiation transfer equations under the constraints of hydrostatic, radiative and statistical equilibrium (non-LTE). We outline the basic idea of the Accelerated Lambda Iteration (ALI) technique and statistical methods which finally allow the construction of non-LTE model atmospheres considering the influence of millions of metal absorption lines. Some applications of the new models are presented. (C) 1999 Elsevier Science B.V. All rights reserved.

引用

页码：65 / 93

页数：29

共 47 条

[11]

Haas S, 1996, ASTRON ASTROPHYS, V311, P669

[12]

HAAS S, 1997, THESIS U ERLANGEN NU

[13]

HAMANN WR, 1991, NATO ADV SCI I C-MAT, V341, P69

[14] MULTILEVEL NON-LTE RADIATIVE-TRANSFER IN EXPANDING SHELLS [J].

HAUSCHILDT, PH .

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 1993, 50 (03) :301-318

[15] Numerical solution of the expanding stellar atmosphere problem [J].

Hauschildt, PH ;

Baron, E .

JOURNAL OF COMPUTATIONAL AND APPLIED MATHEMATICS, 1999, 109 (1-2) :41-63

[16] NON-LTE LINE-BLANKETED MODEL ATMOSPHERES OF HOT STARS .1. HYBRID COMPLETE LINEARIZATION ACCELERATED LAMBDA-ITERATION METHOD [J].

HUBENY, I ;

LANZ, T .

ASTROPHYSICAL JOURNAL, 1995, 439 (02) :875-904

[17] A COMPUTER-PROGRAM FOR CALCULATING NON-LTE MODEL STELLAR ATMOSPHERES [J].

HUBENY, I .

COMPUTER PHYSICS COMMUNICATIONS, 1988, 52 (01) :103-132

[18]

HUBENY I, 1992, ASTRON ASTROPHYS, V262, P501

[19]

HUBENY I, 1994, A A, V282, P157

[20]

HUBENY I, 1992, LECTURE NOTES PHYSIC, V401, P377

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