ON THE ASTROPHYSICAL INTERPRETATION OF ISOTOPE ANOMALIES IN METEORITIC SIC GRAINS

被引：145

作者：

GALLINO, R

BUSSO, M

PICCHIO, G

RAITERI, CM

机构：

[1] OSSERV ASTRON TORINO,I-10025 PINO TORINESE,ITALY

[2] SCUOLA INT SUPER STUDI AVANZATI,I-34014 TRIESTE,ITALY

来源：

NATURE | 1990年 / 348卷 / 6299期

关键词：

D O I：

10.1038/348298a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Meteoritic silicon carbide grains, formed in the winds from carbon stars, contain noble gases and other species whose elemental and isotopic abundances are a probe of stellar nucleosynthesis. Theoretical models of carbon stars can explain a variety of measured abundances, in particular the range of krypton isotope ratios and the excess 22Ne found in the grains. © 1990 Nature Publishing Group.

引用

页码：298 / 302

页数：5

共 33 条

[21] THE ASYMPTOTIC GIANT BRANCH EVOLUTION OF 1.0-3.0 M. STARS AS A FUNCTION OF MASS AND COMPOSITION [J].