EFFECT OF RESONANCE-LINE TRANSFER ON HYDROGEN IONIZATION

被引：5

作者：

BEEBE, HA

MILKEY, RW

机构：

来源：

关键词：

D O I：

10.1086/180903

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L111 / &

共 9 条

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[3] AUER LH, 1969, ASTROPHYS J, V145, P784
[4] HARVARD-SMITHSONIAN REFERENCE ATMOSPHERE
GINGERICH, O
NOYES, RW
KALKOFEN, W
CUNY, Y
[J]. SOLAR PHYSICS, 1971, 18 (03) : 347 - +
[5] NEUTRAL HELIUM LINES AND DEPARTURES FROM LTE IN HOT STARS
JOHNSON, HR
POLAND, AI
[J]. JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 1969, 9 (08) : 1151 - &
[6] STATISTICAL-EQUILIBRIUM MODEL ATMOSPHERES FOR EARLY-TYPE STARS .2. HYDROGEN CONTINUA
MIHALAS, D
[J]. ASTROPHYSICAL JOURNAL, 1967, 149 (1P1) : 169 - &
[7] SOLAR LYMAN CONTINUUM AND STRUCTURE OF SOLAR CHROMOSPHERE
NOYES, RW
KALKOFEN, W
[J]. SOLAR PHYSICS, 1970, 15 (01) : 120 - &
[8] POLAND AI, 1969, THESIS INDIANA U
[9] ZIRIN H, 1966, SOLAR ATMOSPHERE, P309