APPROXIMATE SOLUTIONS OF RADIATIVE-TRANSFER IN DUSTY NEBULAE .2. HYDROGEN AND HELIUM

被引:5
作者
DANA, RA
PETROSIAN, V
机构
[1] STANFORD UNIV,INST PLASMA RES,STANFORD,CA 94305
[2] STANFORD UNIV,DEPT APPL PHYS,STANFORD,CA 94305
[3] NASA, AMES RES CTR,MOFFETT FIELD,CA 94035
关键词
D O I
10.1086/154614
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:354 / 364
页数:11
相关论文
共 7 条
[1]   NON-LTE MODEL ATMOSPHERES .7. HYDROGEN AND HELIUM SPECTRA OF O STARS [J].
AUER, LH ;
MIHALAS, D .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1972, 24 :193-&
[2]   RADIATIVE RECOMBINATION OF HE [J].
BURGESS, A ;
SEATON, MJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1960, 121 (05) :471-473
[3]   THE IONIZATION STRUCTURE OF PLANETARY NEBULAE .3. THE IONIZATION OF HELIUM [J].
HUMMER, DG ;
SEATON, MJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1964, 127 (3-4) :217-240
[5]  
Petrosian V., 1973, International Astronomical Union Symposium No.52, Interstellar Dust and Related Topics, P445
[6]   APPROXIMATE SOLUTIONS OF RADIATIVE-TRANSFER IN DUSTY NEBULAE .1. PURE HYDROGEN NEBULAE [J].
PETROSIAN, V ;
DANA, RA .
ASTROPHYSICAL JOURNAL, 1975, 196 (03) :733-744
[7]  
PETROSIAN V, 1974, H 2 REGIONS GALACTIC, P173