QUALITATIVE EXPLANATIONS OF RED GIANT FORMATION

被引:4
作者
BHASKAR, R
NIGAM, A
机构
[1] IBM Thomas J. Watson Research Center, Yorktown Heights, NY 10598
关键词
STARS; INTERIORS; LATE-TYPE;
D O I
10.1086/170003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent research on giant formation has focused on the need for qualitative explanations. The explanations have the following general, qualitative form: the polytrope n assumes a certain value, that makes d ln r/d ln z take on a very large value; large increases in r can then be explained in terms of small changes in the variable z. This form is applicable to all the explanations current in the literature-they all have (1) either implicitly or explicitly, both a hydrostatic component and a luminosity-opacity component, and (2) a reliance on singular solutions. Dimensional analysis reveals that power laws that assume the polytrope n --> 5 are identical in both the hydrostatic and luminosity-based explanations.
引用
收藏
页码:592 / 596
页数:5
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