ON THE STABILITY OF STELLAR WINDS FROM EARLY-TYPE STARS

被引：12

作者：

KAHN, FD

机构：

来源：

关键词：

D O I：

10.1093/mnras/196.3.641

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：641 / 657

页数：17

共 13 条

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[2] STELLAR WINDS
CASSINELLI, JP
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[3] CHANDRASEKHAR S, 1950, RAD TRANSFER, pCH5
[4] de Jager C., 1979, Astronomy and Astrophysics, V79, pL28
[5] HARNDEN FR, 1979, ASTROPHYS J, V234, pL51, DOI 10.1086/183107
[6] Hutchings J. B., 1979, IAU S, P3
[7] MASS LOSS BY HOT STARS
LUCY, LB
SOLOMON, PM
[J]. ASTROPHYSICAL JOURNAL, 1970, 159 (03) : 879 - &
[8] FORMATION OF RESONANCE LINES IN EXTENDED AND EXPANDING ATMOSPHERES
LUCY, LB
[J]. ASTROPHYSICAL JOURNAL, 1971, 163 (01) : 95 - &
[9] LUCY LB, 1981, PREPRINT
[10] RADIATIVE AMPLIFICATION OF SOUND-WAVES IN THE WINDS OF O-STAR AND B-STAR
MACGREGOR, KB
HARTMANN, L
RAYMOND, JC
[J]. ASTROPHYSICAL JOURNAL, 1979, 231 (02) : 514 - 523