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湍流应力对AGB星物质损失率作用的初步探讨
引用本文:汪志云,陈培杰. 湍流应力对AGB星物质损失率作用的初步探讨[J]. 广西民族大学学报, 2007, 13(2): 79-82
作者姓名:汪志云  陈培杰
作者单位:襄樊学院物理与电子信息技术系 湖北襄樊441053
摘    要:通过分析8M⊙和2.8M⊙早期AGB星外部湍流应力与引力的比值在几个演化点上随质量的分布,发现在恒星外部存在一个湍流应力与引力的比值能达到几十的区域,该区域的位置随演化时间的变化而变化,此位置以外的壳层质量随时间的变化规律与Nieuwenhuijzen H.et.Al给出的恒星质量损失率的变化规律完全相同.在此基础上拟合出早期AGB星的质量损失率与出现最大湍流应力位置以外的壳层质量之间的关系式,提出湍流作用对星风的主要影响应体现在湍流作用大的区域在恒星外壳中的位置.

关 键 词:AGB星  湍流  星风损失率
文章编号:1673-8462(2007)02-0079-04
修稿时间:2007-04-08

Discussion on Relationship between Turbulent stress and Mass Loss Rates of AGB Star
WANG zhi-yun,CHEN Pei-jie. Discussion on Relationship between Turbulent stress and Mass Loss Rates of AGB Star[J]. Journal of Guangxi University For Nationalities, 2007, 13(2): 79-82
Authors:WANG zhi-yun  CHEN Pei-jie
Affiliation:Xiangfan University.Xiangfan.441053 China
Abstract:According to Analyzing the distribution of the ratio of the turbulent stress to gravitation of pro--AGB with 2.8Mo and 8Mo on several evolution point, an area which the turbulent stress is several times as big as gravitation outward star is found. The position of this area is changed with the evolution time, and the Variety of mass outward this position is the same as the mass loss rates that is result of calculation with formulae of Nieuwenhuijzen. H. et. Al giving. We educe the formulae between the mass outward the position of appearing the maximal turbulent stress and the mass loss rates of pro--AGB, and present the primary Contribution of Turbulent Effect on stellar wind is the position of the area of existing larger turbulent stress.
Keywords:stellar structure and evolution  AGB star  turbulent
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