JOURNAL ARTICLE
星系螺旋结构三维密度波的流体动力学理论
Year: 1980 Journal: Chinese Science Bulletin (Chinese Version) Vol: 25 (1)Pages: 47-48 Publisher: Science China Press
Abstract
<正> 盘状星系螺旋结构的本质与起源是半个多世纪以来一直为天文学及天体物理学界所注目的重大难题。在近十五年来,由林家翘所创建的密度波理论,在揭示星系螺旋结构的动力学机制上取得了很大的成功,但是林家翘的理论仍有一定的局限性,他将
Keywords:
Computer science
Metrics
0
Cited By
0.00
FWCI (Field Weighted Citation Impact)
0
Refs
Citation Normalized Percentile
Is in top 1%
Is in top 10%
Topics
Related Documents
JOURNAL ARTICLE
星系螺旋结构三维密度波的流体动力学理论(I)——局部解及局部Jeans稳定性的讨论
Journal: 力学学报 Year: 1980 Vol: 16 (3)Pages: 232-242
JOURNAL ARTICLE
行星际高密度结构的磁流体动力学特性
Journal: Science in China Series A-Mathematics Physics Astronomy & Technological Science (in Chinese) Year: 1989 Vol: 19 (5)Pages: 502-508
JOURNAL ARTICLE
密度波理论中星系激波的性质
Journal: Chinese Science Bulletin (Chinese Version) Year: 1977 Vol: 22 (2)Pages: 79-83
JOURNAL ARTICLE
盘状星系松卷旋密度波引力不稳定性的恒星动力学研究
Journal: Chinese Science Bulletin (Chinese Version) Year: 1980 Vol: 25 (2)Pages: 77-81
JOURNAL ARTICLE
基于流体动力学理论的颗粒物质本构关系
Journal: Chinese Science Bulletin (Chinese Version) Year: 2009 Vol: 54 (11)Pages: 1504-1510