VELOCITY-DEPENDENT SOURCE FUNCTION IN RADIATIVE-TRANSFER THEORY

被引：7

作者：

CANNON, CJ ^{[1
]}

CRAM, LE ^{[1
]}

机构：

[1] UNIV SYDNEY,DEPT APPL MATH,SYDNEY 2006,NEW S WALES,AUSTRALIA

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 1974年 / 14卷 / 02期

关键词：

D O I：

10.1016/0022-4073(74)90002-8

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

引用

页码：93 / 99

页数：7

共 18 条

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[6]

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[7]

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[8] LINE FORMATION IN PULSATING VARIABLE STARS [J].

KALKOFEN, W ;

WHITNEY, CA .

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[9]

KALKOFEN W, 1970, NBS332 SPEC PUB

[10]

KOGURE T, 1962, P ASTRON SOC JAPAN, V247

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