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![Dynamics of Young Star Clusters and Associations: Saas-Fee Advanced Course 42. Swiss Society for Astrophysics and Astronomy by Cathie Clarke, Robert D. Mathieu, Iain Neill Reid](https://558130.bdp32.group/rails/active_storage/representations/redirect/eyJfcmFpbHMiOnsibWVzc2FnZSI6IkJBaHBBNW0va2c9PSIsImV4cCI6bnVsbCwicHVyIjoiYmxvYl9pZCJ9fQ==--5eec6ef1e45d868b9c5f05d95d06cd7a16406875/eyJfcmFpbHMiOnsibWVzc2FnZSI6IkJBaDdCem9MWm05eWJXRjBTU0lJYW5CbkJqb0dSVlE2RkhKbGMybDZaVjkwYjE5c2FXMXBkRnNIYVFJc0FXa0M5QUU9IiwiZXhwIjpudWxsLCJwdXIiOiJ2YXJpYXRpb24ifX0=--038335c90cf75c275ae4d36968ac417dc4a0a3e3/Dynamics%20of%20Young%20Star%20Clusters%20and%20Associations-%20Saas-Fee%20Advanced%20Course%2042.%20Swiss%20Society%20for%20Astrophysics%20and%20Astronomy.jpg)
348 pages • missing pub info (editions)
ISBN/UID: 9783662514603
Format: Paperback
Language: English
Publisher: Springer
Publication date: 23 August 2016
Description
Where do most stars (and the planetary systems that surround them) in the Milky Way form? What determines whether a young star cluster remains bound (such as an open or globular cluster), or disperses to join the field stars in the disc of the Gal...
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![Dynamics of Young Star Clusters and Associations: Saas-Fee Advanced Course 42. Swiss Society for Astrophysics and Astronomy by Cathie Clarke, Robert D. Mathieu, Iain Neill Reid](https://558130.bdp32.group/rails/active_storage/representations/redirect/eyJfcmFpbHMiOnsibWVzc2FnZSI6IkJBaHBBNW0va2c9PSIsImV4cCI6bnVsbCwicHVyIjoiYmxvYl9pZCJ9fQ==--5eec6ef1e45d868b9c5f05d95d06cd7a16406875/eyJfcmFpbHMiOnsibWVzc2FnZSI6IkJBaDdCem9MWm05eWJXRjBTU0lJYW5CbkJqb0dSVlE2RkhKbGMybDZaVjkwYjE5c2FXMXBkRnNIYVFJc0FXa0M5QUU9IiwiZXhwIjpudWxsLCJwdXIiOiJ2YXJpYXRpb24ifX0=--038335c90cf75c275ae4d36968ac417dc4a0a3e3/Dynamics%20of%20Young%20Star%20Clusters%20and%20Associations-%20Saas-Fee%20Advanced%20Course%2042.%20Swiss%20Society%20for%20Astrophysics%20and%20Astronomy.jpg)
348 pages • missing pub info (editions)
ISBN/UID: 9783662514603
Format: Paperback
Language: English
Publisher: Springer
Publication date: 23 August 2016
Description
Where do most stars (and the planetary systems that surround them) in the Milky Way form? What determines whether a young star cluster remains bound (such as an open or globular cluster), or disperses to join the field stars in the disc of the Gal...