On gas dynamical models of galaxies

Cai Shu-tang
{"title":"On gas dynamical models of galaxies","authors":"Cai Shu-tang","doi":"10.1016/0146-6364(80)90052-3","DOIUrl":null,"url":null,"abstract":"<div><p>This paper discussed the range of applicability of the gas dynamical equations used in gas dynamical models. It is pointed out that (1), when dealing with gravitational collapse, the law of mass conservation and the equation of continuity are inapplicable if the reaction energies are large. (2) The presence of turbulence only affects the basic-state motion. If the basic-state motion is given and if we neglect higher-order small quantities and if we make certain simplifying assumptions, then the equations for small perturbations are of the same form as in the absence of turbulence. The equations used by C.C. Lin and his coworkers are precisely equations for small perturbations, hence Lin's theory still holds even if there is turbulence. If we wish to go to the next approximation, then we must, in general, take account of turbulence.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"1980-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90052-3","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0146636480900523","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

This paper discussed the range of applicability of the gas dynamical equations used in gas dynamical models. It is pointed out that (1), when dealing with gravitational collapse, the law of mass conservation and the equation of continuity are inapplicable if the reaction energies are large. (2) The presence of turbulence only affects the basic-state motion. If the basic-state motion is given and if we neglect higher-order small quantities and if we make certain simplifying assumptions, then the equations for small perturbations are of the same form as in the absence of turbulence. The equations used by C.C. Lin and his coworkers are precisely equations for small perturbations, hence Lin's theory still holds even if there is turbulence. If we wish to go to the next approximation, then we must, in general, take account of turbulence.

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
关于星系的气体动力学模型
本文讨论了用于气体动力学模型的气体动力学方程的适用范围。指出(1)在处理引力坍缩时,当反应能量较大时,质量守恒定律和连续性方程不适用。(2)湍流的存在只影响基态运动。如果基态运动是给定的,如果我们忽略高阶小量,如果我们做一些简化的假设,那么小扰动的方程和没有湍流时的方程形式是一样的。C.C. Lin和他的同事所使用的方程正是小扰动的方程,因此即使存在湍流,Lin的理论仍然成立。如果我们希望得到下一个近似,那么我们通常必须考虑湍流。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
自引率
0.00%
发文量
0
期刊最新文献
Subject index Errata Author index Supernova remnants of known age and X-radiation The effect of an ellipsoidal distribution of star velocities on galactic density waves
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1