STELLAR ATMOSPHERES PROBLEM

被引：56

作者：

AUER, LH

机构：

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 1971年 / 11卷 / 06期

关键词：

D O I：

10.1016/0022-4073(71)90039-2

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

引用

页码：573 / +

页数：1

共 29 条

[1]

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[3] ON USE OF VARIABLE EDDINGTON FACTORS IN NON-LTE STELLAR ATMOSPHERES COMPUTATIONS [J].

AUER, LH ;

MIHALAS, D .

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[4] NON-LTE MODEL ATMOSPHERES .I. RADIATIVE EQUILIBRIUM MODELS WITH LYMAN-ALPHA [J].

AUER, LH ;

MIHALAS, D .

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[5] SOLUTION OF TRANSFER EQUATIONS SUBJECT TO CONSTRAINT OF RADIATIVE EQUILIBRIUM [J].

AUER, LH ;

MIHALAS, D .

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[6] NON-LTE MODEL ATMOSPHERES .3. A COMPLETE-LINEARIZATION METHOD [J].

AUER, LH ;

MIHALAS, D .

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[7] SOLUTION OF NON-LTE TRANSFER PROBLEMS [J].

AVRETT, EH .

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 1971, 11 (06) :511-+

[8] TEMPERATURE DISTRIBUTION IN A STELLAR ATMOSPHERE [J].

AVRETT, EH ;

KROOK, M .

ASTROPHYSICAL JOURNAL, 1963, 137 (03) :874-&

[9]

BOHM KH, 1954, Z ASTROPHYS, V34, P182

[10] A BASIC LIMIT OF THE INFORMATION CONTAINED IN CENTER-TO-LIMB OBSERVATIONS [J].

BOHM, KH .

ASTROPHYSICAL JOURNAL, 1961, 134 (01) :264-267

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