ANALYSIS OF MN-I LINES IN THE SOLAR SPECTRUM USING ACCURATE OSCILLATOR-STRENGTHS

被引：19

作者：

BOOTH, AJ ^{[1
]}

BLACKWELL, DE ^{[1
]}

SHALLIS, MJ ^{[1
]}

机构：

[1] OXFORD UNIV,DEPT EXTERNAL STUDIES,OXFORD OX1 2AJ,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1984年 / 209卷 / 01期

关键词：

D O I：

10.1093/mnras/209.1.77

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：77 / 81

页数：5

共 28 条

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[2] COMPUTATION OF OSCILLATOR-STRENGTHS BY A SEMIEMPIRICAL METHOD FOR SOME ELEMENTS OF IRON-GROUP AND THEIR SOLAR PHOTOSPHERIC ABUNDANCE .3. RESULTS FOR MN-1 [J].

BIEMONT, E .

SOLAR PHYSICS, 1975, 44 (02) :269-273

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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1982, 199 (01) :37-42

[4]

BLACKWELL DE, 1980, ASTRON ASTROPHYS, V81, P340

[5] INTERPRETATION OF THE SOLAR SPECTRUM 300-900 NM .2. FE-I LINES OF EXCITATION POTENTIAL 0.00-1.01EV - USE OF NEW OSCILLATOR-STRENGTHS OF 0.5-PERCENT ACCURACY [J].

BLACKWELL, DE ;

SHALLIS, MJ .

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[6]

BLACKWELL DE, 1984, ASTRON ASTROPHYS, V132, P236

[7] SOLAR ABUNDANCE OF MANGANESE [J].

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[8] THE EFFECT OF HYPERFINE-STRUCTURE ON STELLAR ABUNDANCE ANALYSIS [J].

BOOTH, AJ ;

BLACKWELL, DE .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1983, 204 (02) :777-781

[9] HYPERFINE-STRUCTURE MEASUREMENTS FOR LINES OF ASTROPHYSICAL INTEREST IN MN-I [J].

BOOTH, AJ ;

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WELLS, M .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1983, 205 (01) :191-205

[10]

BOOTH AJ, 1982, THESIS U OXFORD

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