ARE S-ELEMENTS REALLY PRODUCED DURING THERMAL PULSES IN INTERMEDIATE-MASS STARS

被引:52
作者
BUSSO, M
PICCHIO, G
GALLINO, R
CHIEFFI, A
机构
[1] UNIV TORINO,IST FIS GEN,I-10100 TORINO,ITALY
[2] CNR,IST ASTROFIS SPAZIALE,FRASCATI,ITALY
关键词
D O I
10.1086/166081
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:196 / 207
页数:12
相关论文
共 66 条
[21]   A DIFFICULTY WITH NE-22 AS THE NEUTRON SOURCE FOR THE SOLAR-SYSTEM S-PROCESS [J].
DESPAIN, KH .
ASTROPHYSICAL JOURNAL, 1980, 236 (03) :L165-L168
[22]   THERMONUCLEAR REACTION-RATES .2. [J].
FOWLER, WA ;
CAUGHLAN, GR ;
ZIMMERMAN, BA .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1975, 13 :69-112
[23]  
FUELLER GM, 1982, AP J SUPPL, V48, P279
[24]  
GALLINO R, 1985, NUCLEI STARS, P309
[25]  
HABING HJ, 1987, P NATO ADV STUDY I G, P173
[26]   THERMONUCLEAR REACTION-RATES, .3. [J].
HARRIS, MJ ;
FOWLER, WA ;
CAUGHLAN, GR ;
ZIMMERMAN, BA .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1983, 21 :165-176
[27]  
HOLLOWELL D, 1987, P WORKSHOP LATE STAG, P239
[28]   THERMAL CONDUCTION BY ELECTRONS IN STELLAR MATTER [J].
HUBBARD, WB ;
LAMPE, M .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1969, 18 (163) :297-&
[29]   SURFACE COMPOSITION OF THERMALLY PULSING STARS OF HIGH LUMINOSITY AND ON CONTRIBUTION OF SUCH STARS TO ELEMENT ENRICHMENT OF INTER-STELLAR MEDIUM [J].
IBEN, I ;
TRURAN, JW .
ASTROPHYSICAL JOURNAL, 1978, 220 (03) :980-995
[30]   THERMAL PULSE AND INTERPULSE PROPERTIES OF INTERMEDIATE-MASS STELLAR MODELS WITH CARBON-OXYGEN CORES OF MASS 0.96, 1.16, AND 1.36M. [J].
IBEN, I .
ASTROPHYSICAL JOURNAL, 1977, 217 (03) :788-798