RELATIVE ABUNDANCES IN METAL-POOR STARS .2. CARBON-TO-IRON RATIO

被引：39
作者：
PETERSON, RC
SNEDEN, C
机构：
[1] LOCKHEED AIRCRAFT CORP,PALO ALTO RES LAB,PALO ALTO,CA 94304
[2] UNIV WASHINGTON,DEPT ASTRON,SEATTLE,WA 98195
[3] UNIV WYOMING,DEPT PHYS & ASTRON,LARAMIE,WY 82070
来源：
ASTROPHYSICAL JOURNAL | 1978年 / 225卷 / 03期
关键词：
D O I：
10.1086/156557
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：913 / 918
页数：6
相关论文
共 55 条
[1]  
[Anonymous], 1973, PHOTOMETRIC ATLAS SO
[2]   BULK YIELDS OF NUCLEOSYNTHESIS FROM MASSIVE STARS [J].
ARNETT, WD .
ASTROPHYSICAL JOURNAL, 1978, 219 (03) :1008-1016
[3]   EXPLOSIVE NUCLEOSYNTHESIS IN STARS [J].
ARNETT, WD .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1973, 11 :73-94
[4]   EXPLOSIVE NUCLEOSYNTHESIS IN STARS [J].
ARNETT, WD ;
CLAYTON, DD .
NATURE, 1970, 227 (5260) :780-&
[5]  
AUDOUZE J, 1975, ASTRON ASTROPHYS, V43, P71
[6]   CHEMICAL EVOLUTION OF GALAXIES [J].
AUDOUZE, J ;
TINSLEY, BM .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1976, 14 :43-79
[7]  
BASCHEK B, 1962, Z ASTROPHYS, V56, P207
[8]   CARBON ABUNDANCES IN G-DWARFS [J].
BELL, RA ;
BRANCH, D .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 175 (01) :25-32
[9]   INTERPRETATION OF SOLAR SPECTRUM 300 NM TO 900 NM .1. FE I LINES OF EXCITATION POTENTIAL 0.00 EV-0.12 EV MICROTURBULENCE, DAMPING, ABUNDANCE, TESTS OF OSCILLATOR-STRENGTHS [J].
BLACKWELL, DE ;
IBBETSON, PA ;
PETFORD, AD ;
WILLIS, RB .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 177 (01) :227-245
[10]   SYNTHESIS OF THE ELEMENTS IN STARS [J].
BURBIDGE, EM ;
BURBIDGE, GR ;
FOWLER, WA ;
HOYLE, F .
REVIEWS OF MODERN PHYSICS, 1957, 29 (04) :547-650
123456