PMO OpenIR  > 院士文集  > 熊大闰
湍动对流与变星脉动稳定性
熊大闰
1980
Source Publication中国科学
ISSN1006-9232
Volume0Issue:4Pages:347-355
Abstract本文利用文献[1]所发展的随时间变化的对流理论,研究了径向脉动运动同对流的耦合.由天琴座RR型变星和仙王座δ型变星模型的线性非绝热脉动计算表明,当考虑了对流与脉动的热力学耦合后,我们将可以确定脉动不稳定区红端边界的位置.并可望去解释长周期变星.以及晚型红巨星和超巨星光的变化性.
Keyword对流区 仙王座 天琴座 径向脉动 湍动 长周期变星 电离区 时间变化 红巨星 有效温度
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/11167
Collection院士文集_熊大闰
Recommended Citation
GB/T 7714
熊大闰. 湍动对流与变星脉动稳定性[J]. 中国科学,1980,0(4):347-355.
APA 熊大闰.(1980).湍动对流与变星脉动稳定性.中国科学,0(4),347-355.
MLA 熊大闰."湍动对流与变星脉动稳定性".中国科学 0.4(1980):347-355.
Files in This Item:
File Name/Size DocType Version Access License
1980248湍动对流与变星脉动稳定性1(958KB) 开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[熊大闰]'s Articles
Baidu academic
Similar articles in Baidu academic
[熊大闰]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[熊大闰]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 1980248湍动对流与变星脉动稳定性100006306099.pdf
Format: Adobe PDF
This file does not support browsing at this time
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.