EFFECTS OF NON-CONSTANT SCATTERING OPACITY ON MODELS FOR MASSIVE STARS INITIALLY COMPOSED OF PURE HYDROGEN

被引：6

作者：

BOURY, A

机构：

来源：

ASTROPHYSICAL JOURNAL | 1964年 / 140卷 / 03期

关键词：

D O I：

10.1086/148032

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：1322 / &

相关论文

共 10 条

[1] BOURY A, 1960, B SOC ROY SCI LIEGE, V29, P306
[2] BOURY A, 1963, ANN AP, V26, P354
[3] CHANDRASEKHAR S, 1939, STELLAR STRUCTURE, P56
[4] MODELS OF MASSIVE PURE HYDROGEN STARS
EZER, D
[J]. ASTROPHYSICAL JOURNAL, 1961, 133 (01) : 159 - 165
[5] COMPLETION OF THE PROTON-PROTON REACTION CHAIN AND THE POSSIBILITY OF ENERGETIC NEUTRINO EMISSION BY HOT STARS
FOWLER, WA
[J]. ASTROPHYSICAL JOURNAL, 1958, 127 (03) : 551 - 556
[6] FOWLER WA, 1960, 9 LIEG S MEM SOC R 5, V3, P207
[7] LEVEE RD, 1960, 9 LIEG S MEM SOC R 5, V3, P298
[8] THE OPACITY AT HIGH TEMPERATURES DUE TO COMPTON SCATTERING
SAMPSON, DH
[J]. ASTROPHYSICAL JOURNAL, 1959, 129 (03) : 734 - 751
[9] EVOLUTION OF VERY MASSIVE STARS
SCHWARZSCHILD, M
HARM, R
[J]. ASTROPHYSICAL JOURNAL, 1958, 128 (02) : 348 - 360
[10] ON THE MAXIMUM MASS OF STABLE STARS
SCHWARZSCHILD, M
HARM, R
[J]. ASTROPHYSICAL JOURNAL, 1959, 129 (03) : 637 - 646