LOW-MASS STARS .2. THE CORE MASS-LUMINOSITY RELATIONS

被引：103

作者：

BOOTHROYD, AI ^{[1
]}

SACKMANN, IJ ^{[1
]}

机构：

[1] CALTECH,KELLOGG RADIAT LAB,PASADENA,CA 91125

来源：

ASTROPHYSICAL JOURNAL | 1988年 / 328卷 / 02期

关键词：

D O I：

10.1086/166322

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：641 / 652

页数：12

共 30 条

[1] THE EXTENDED GIANT BRANCHES OF INTERMEDIATE AGE GLOBULAR-CLUSTERS IN THE MAGELLANIC CLOUDS .4.
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[2] LOW-MASS STARS .3. LOW-MASS STARS WITH STEADY MASS-LOSS - UP TO THE ASYMPTOTIC GIANT BRANCH AND THROUGH THE FINAL THERMAL PULSES
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[3] LOW-MASS STARS .1. FLASH-DRIVEN LUMINOSITY AND RADIUS VARIATIONS
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[4] THERMONUCLEAR REACTION-RATES .2.
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[7] FURTHER ADVENTURES OF A THERMALLY PULSING STAR
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[8] THERMAL PULSES - P-CAPTURE, ALPHA-CAPTURE, S-PROCESS NUCLEOSYNTHESIS - CONVECTIVE MIXING IN A STAR OF INTERMEDIATE MASS
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[J]. ASTROPHYSICAL JOURNAL, 1975, 196 (02) : 525 - 547
[9] SURFACE COMPOSITION OF THERMALLY PULSING STARS OF HIGH LUMINOSITY AND ON CONTRIBUTION OF SUCH STARS TO ELEMENT ENRICHMENT OF INTER-STELLAR MEDIUM
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[J]. ASTROPHYSICAL JOURNAL, 1978, 220 (03) : 980 - 995
[10] THERMAL PULSE AND INTERPULSE PROPERTIES OF INTERMEDIATE-MASS STELLAR MODELS WITH CARBON-OXYGEN CORES OF MASS 0.96, 1.16, AND 1.36M.
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