NON-LTE CALCULATIONS OF AL-III LINE STRENGTHS IN EARLY-TYPE STARS

被引:25
作者
DUFTON, PL [1 ]
BROWN, PJF [1 ]
LENNON, DJ [1 ]
LYNASGRAY, AE [1 ]
机构
[1] UNIV LONDON UNIV COLL,DEPT PHYS & ASTRON,LONDON WC1E 6BT,ENGLAND
关键词
D O I
10.1093/mnras/222.4.713
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:713 / 718
页数:6
相关论文
共 28 条
[11]   THE NITROGEN TO HYDROGEN ABUNDANCE IN MAIN-SEQUENCE B-TYPE STARS [J].
DUFTON, PL ;
KANE, L ;
MCKEITH, CD .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1981, 194 (01) :85-93
[12]  
DUFTON PL, 1980, ASTRON ASTROPHYS, V81, P8
[13]  
DUFTON PL, 1981, ASTRON ASTROPHYS, V95, P24
[14]  
DUFTON PL, 1979, ASTRON ASTROPHYS, V73, P203
[15]  
DUFTON PL, 1985, UNPUB J PHYS B
[16]  
Griem H. R., 1974, SPECTRAL LINE BROADE
[17]  
HOWARTH ID, 1984, 50 STARL US NOT
[18]  
Jefferies J.T., 1968, SPECTRAL LINE FORMAT
[19]  
Konjevic N., 1976, Journal of Physical and Chemical Reference Data, V5, P259, DOI 10.1063/1.555533
[20]  
KUDRITZKI RP, 1976, ASTRON ASTROPHYS, V52, P11