CHEMICAL EVOLUTION IN AN INHOMOGENEOUS INTERSTELLAR-MEDIUM

被引:0
|
作者
WILMES, M [1 ]
KOPPEN, J [1 ]
机构
[1] CHRISTIAN ALBRECHTS UNIV KIEL, INST THEORET PHYS & STERNWARTE, D-24118 KIEL, GERMANY
关键词
GALAXY; ABUNDANCES; EVOLUTION; NUCLEOSYNTHESIS;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the chemical evolution of secondary and primary elements in a model which allows for inhomogeneities in the interstellar medium due to incomplete mixing of stellar ejecta, and a star formation localized in time and space. The average abundances are the same as the single value obtained from homogeneous models. The inhomogeneous star formation causes a scatter of the abundances of the ISM. Incomplete mixing has a strong influence on the relation between nitrogen and oxygen, giving rise to flatter N/O-O/H relations, thus mimicking a primary contribution to the nitrogen synthesis. Comparison with observational data from the Galaxy and external galaxies indicates that the probability of star formation is about T = 0.1, in accord with the scatter of stellar metallicities which indicates that the degree of chemical inhomogeneity of the interstellar gas is indeed rather small.
引用
收藏
页码:47 / 56
页数:10
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