MICROTURBULENCE IN A STARS AS DERIVED FROM LINE PROFILES

被引:21
作者
SMITH, MA [1 ]
机构
[1] LICK OBSERV,BOARD STUDIES ASTRON & ASTROPHYS,SANTA CRUZ,CA 95060
关键词
D O I
10.1086/152127
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:159 / 175
页数:17
相关论文
共 38 条
[1]   LINE BROADENING IN HIGH-LUMINOSITY STARS .2. LESS LUMINOUS SUPERGIANTS [J].
ABT, HA .
ASTROPHYSICAL JOURNAL, 1958, 127 (03) :658-666
[2]  
ABT HA, 1972, ASTROPHYS J, V171, P259, DOI 10.1086/151278
[3]   FE I IONIZATION AND EXCITATION EQUILIBRIUM IN SOLAR ATMOSPHERE [J].
ATHAY, RG ;
LITES, BW .
ASTROPHYSICAL JOURNAL, 1972, 176 (03) :809-&
[4]   THEORETICAL LINE INTENSITIES .6. MILNE-EDDINGTON CURVES OF GROWTH FOR NON-COHERENT SCATTERING [J].
ATHAY, RG ;
SKUMANIC.A .
ASTROPHYSICAL JOURNAL, 1968, 152 (1P1) :211-&
[5]  
BASCHEK B, 1969, ASTRON ASTROPHYS, V2, P240
[6]  
BATTEN AH, 1967, PUBL DOM ASTROPHYS O, V13, P119
[7]  
BOLTON CT, 1971, ASTRON ASTROPHYS, V14, P233
[8]  
CARBON D, 1969, 3 P HARV SMITHS C ST
[9]  
CAYRELDESTROBEL G, 1968, ANN ASTROPHYS, V31, P43
[10]  
CHAFFEE FH, 1970, ASTRON ASTROPHYS, V4, P291