A VARIATIONAL METHOD FOR IMPROVING MODEL STELLAR ATMOSPHERES

被引：6

作者：

PRZYBYLSKI, A

机构：

来源：

关键词：

D O I：

10.1093/mnras/115.6.650

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：650 / 660

页数：11

共 14 条

[1] MCDONALD KJ, 1953, PUBL DOM AP OBS, V9, P269
[2] Michard R., 1949, Annales d'Astrophysique, V12, P291
[3] MILLIGAN JE, 1954, P C STELLAR ATMOSPHE
[4] MODEL SOLAR ATMOSPHERES
MUNCH, G
[J]. ASTROPHYSICAL JOURNAL, 1947, 106 (02) : 217 - 223
[5] NICOLET M, 1951, ANN ASTROPHYS, V14, P249
[6] PECKER JC, 1952, ANN AP, V13, P294
[7] PECKER JC, 1952, ANN AP, V13, P319
[8] PECKER JC, 1952, ANN AP, V13, P433
[9] THE MAXIMUM EFFECT OF CONVECTION IN STELLAR ATMOSPHERES ON THE OBSERVED PROPERTIES OF STELLAR SPECTRA .1.
PRZYBYLSKI, A
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1953, 113 (06) : 683 - 700
[10] THE MAXIMUM EFFECT OF CONVECTION IN STELLAR ATMOSPHERES ON THE OBSERVED PROPERTIES OF STELLAR SPECTRA .2.
PRZYBYLSKI, A
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1954, 114 (04) : 406 - 414