MG II H AND K LINES .2. COMPARISON WITH SYNTHESIZED PROFILES AND CA II K

被引：107

作者：

AYRES, TR ^{[1
]}

LINSKY, JL ^{[1
]}

机构：

[1] UNIV COLORADO NBS JOINT INST LAB ASTROPHYS,BOULDER,CO 80302

来源：

ASTROPHYSICAL JOURNAL | 1976年 / 205卷 / 03期

关键词：

D O I：

10.1086/154344

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：874 / 894

页数：21

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[4] NON-LTE MODEL ATMOSPHERES .3. A COMPLETE-LINEARIZATION METHOD
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[5] AUER LH, 1972, 555 KITT PEAK NAT OB
[6] SEMIEMPIRICAL UPPER PHOTOSPHERE MODELS - SUN (G2V) AND PROCYON (F5IV-V)
AYRES, TR
[J]. ASTROPHYSICAL JOURNAL, 1975, 201 (03) : 799 - 815
[7] STELLAR MODEL CHROMOSPHERES .3. ARCTURUS (K2 III)
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[J]. ASTROPHYSICAL JOURNAL, 1975, 200 (03) : 660 - 674
[8] STELLAR MODEL CHROMOSPHERES .4. FORMATION OF H-EPSILON FEATURE IN SUN (G2V) AND ARCTURUS (K2III)
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[J]. ASTROPHYSICAL JOURNAL, 1975, 201 (01) : 212 - 221
[9] STELLAR MODEL CHROMOSPHERES .2. PROCYON (F5 IV-V)
AYRES, TR
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[J]. ASTROPHYSICAL JOURNAL, 1974, 192 (01) : 93 - 107
[10] AYRES TR, 1975, THESIS U COLORADO

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