STELLAR EVOLUTIONARY MODELS FROM THE ZERO-AGE MAIN-SEQUENCE TO THE 1ST THERMAL PULSE

被引:59
作者
LATTANZIO, JC
机构
[1] Inst. of Geophys. and Planet. Phys., Lawrence Livermore Natl. Lab., L-413, Livermore, CA 94550
关键词
STARS; EVOLUTION; INTERIORS;
D O I
10.1086/191569
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present detailed numerical tabulations of 32 stellar evolutionary sequences extending from either the zero-age main sequence (ZAMS) or the zero-age horizontal branch (ZAHB), and through to the occurrence of thermal pulses on the asymptotic giant branch. The models span a range of 1-3 M. (except for one 4 M. and one 5 M. model) and cover metallicities of Z = 0.02, 0.01, 0.006, 0.003, and 0.001, each with Y = 0.20 and 0.30. These models can be used for various stellar population studies, and as a comparison between rival calculations with different input physics.
引用
收藏
页码:215 / 357
页数:143
相关论文
共 31 条
[1]   THE EVOLUTION OF INTERMEDIATE-MASS STARS FROM THE ZERO-AGE MAIN-SEQUENCE TO THE BASE OF THE ASYMPTOTIC GIANT BRANCH AS A FUNCTION OF MASS AND COMPOSITION [J].
BECKER, SA .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1981, 45 (03) :475-505
[2]   ASYMPTOTIC GIANT BRANCH EVOLUTION OF INTERMEDIATE-MASS STARS AS A FUNCTION OF MASS AND COMPOSITION .1. THROUGH THE 2ND DREDGE-UP PHASE [J].
BECKER, SA ;
IBEN, I .
ASTROPHYSICAL JOURNAL, 1979, 232 (03) :831-853
[4]  
BERTELLI G, 1991, UNPUB
[5]  
BEUDET G, 1971, A A, V13, P209
[6]   LOW-MASS STARS .3. LOW-MASS STARS WITH STEADY MASS-LOSS - UP TO THE ASYMPTOTIC GIANT BRANCH AND THROUGH THE FINAL THERMAL PULSES [J].
BOOTHROYD, AI ;
SACKMANN, IJ .
ASTROPHYSICAL JOURNAL, 1988, 328 (02) :653-670
[7]   LOW-MASS STARS .1. FLASH-DRIVEN LUMINOSITY AND RADIUS VARIATIONS [J].
BOOTHROYD, AI ;
SACKMANN, IJ .
ASTROPHYSICAL JOURNAL, 1988, 328 (02) :632-640
[8]   THE PRODUCTION OF LOW-MASS STARS .4. CARBON STARS [J].
BOOTHROYD, AI ;
SACKMANN, IJ .
ASTROPHYSICAL JOURNAL, 1988, 328 (02) :671-679
[9]  
CASTELLANI V, 1988, PREPRINT
[10]  
CHIEFFI A, 1988, PREPRINT