Titlebook: Symmetries and Dynamics of Star Clusters; Jaroslav Haas Book 2014 Springer International Publishing Switzerland 2014 Dynamics of Star Clus

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書目名稱Symmetries and Dynamics of Star Clusters影響因子(影響力)




書目名稱Symmetries and Dynamics of Star Clusters影響因子(影響力)學(xué)科排名




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書目名稱Symmetries and Dynamics of Star Clusters網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Symmetries and Dynamics of Star Clusters被引頻次




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薄膜

Jaroslav Haasal healing and growth plate disruption, with particular emphasis on bony bridge resection. Our ability to recognize epiphyseal bars has greatly improved. Now, we can better anticipate and recognize growth arres978-1-4757-8153-3978-0-387-21854-0

molest

be effectively treated because of the survival potential. There is a new chapter on abnormal healing and growth plate disruption, with particular emphasis on bony bridge resection. Our ability to recognize epiphyseal bars has greatly improved. Now, we can better anticipate and recognize growth arres

Antagonism

Jaroslav Haasbe effectively treated because of the survival potential. There is a new chapter on abnormal healing and growth plate disruption, with particular emphasis on bony bridge resection. Our ability to recognize epiphyseal bars has greatly improved. Now, we can better anticipate and recognize growth arres

CRASS

Jaroslav Haasbe effectively treated because of the survival potential. There is a new chapter on abnormal healing and growth plate disruption, with particular emphasis on bony bridge resection. Our ability to recognize epiphyseal bars has greatly improved. Now, we can better anticipate and recognize growth arres

resilience

柳樹；枯黃

STENT

2190-5053 y occur in the embedding spherical cluster of old stars. This increases the richness of possible evolution scenarios of the embedding cluster and may lead to effective feeding of supermassive black holes through tidal disruption of stars on extremely eccentric orbits..978-3-319-37857-2978-3-319-03650-2Series ISSN 2190-5053 Series E-ISSN 2190-5061

熄滅

天真

Thin Disc Embedded in Extended Spherically Symmetric Cluster,onable to expect these stellar discs to be embedded in extended spherically symmetric star clusters. Hence, in Chap. 2 of the thesis, we investigate the orbital evolution of an initially thin stellar disc under the gravitational influence of such a spherical star cluster.