CSpace
Post-Newtonian dynamics in dense star clusters: Formation, masses, and merger rates of highly-eccentric black hole binaries
Rodriguez, Carl L.; Amaro-Seoane, Pau; Chatterjee, Sourav; Kremer, Kyle; Rasio, Frederic A.; Samsing, Johan; Ye, Claire S.; Zevin, Michael
2018
Source PublicationPHYSICAL REVIEW D
Volume98Issue:12
Document Type期刊论文
Identifierhttp://ir.amss.ac.cn/handle/2S8OKBNM/33477
Collection中国科学院数学与系统科学研究院
Recommended Citation
GB/T 7714
Rodriguez, Carl L.,Amaro-Seoane, Pau,Chatterjee, Sourav,et al. Post-Newtonian dynamics in dense star clusters: Formation, masses, and merger rates of highly-eccentric black hole binaries[J]. PHYSICAL REVIEW D,2018,98(12).
APA Rodriguez, Carl L..,Amaro-Seoane, Pau.,Chatterjee, Sourav.,Kremer, Kyle.,Rasio, Frederic A..,...&Zevin, Michael.(2018).Post-Newtonian dynamics in dense star clusters: Formation, masses, and merger rates of highly-eccentric black hole binaries.PHYSICAL REVIEW D,98(12).
MLA Rodriguez, Carl L.,et al."Post-Newtonian dynamics in dense star clusters: Formation, masses, and merger rates of highly-eccentric black hole binaries".PHYSICAL REVIEW D 98.12(2018).
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Rodriguez, Carl L.]'s Articles
[Amaro-Seoane, Pau]'s Articles
[Chatterjee, Sourav]'s Articles
Baidu academic
Similar articles in Baidu academic
[Rodriguez, Carl L.]'s Articles
[Amaro-Seoane, Pau]'s Articles
[Chatterjee, Sourav]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Rodriguez, Carl L.]'s Articles
[Amaro-Seoane, Pau]'s Articles
[Chatterjee, Sourav]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

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