Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1779368 | New Astronomy | 2012 | 9 Pages |
Abstract
⺠We have followed hard binary formation in star cluster core collapse. ⺠Unlike standard scenarios, typically many stars are involved simultaneously. ⺠Failure of analytical predictions is related to small core size during core bounce.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Ataru Tanikawa, Piet Hut, Junichiro Makino,