Dynamics of young star clusters and associations : Saas-Fee advanced course 42 /
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| Author / Creator: | Clarke, Cathie J., author. |
|---|---|
| Imprint: | Heidelberg : Springer, 2016. ©2016 |
| Description: | 1 online resource. |
| Language: | English |
| Series: | Saas-fee advanced course ; 42 Saas-Fee advanced course ... lecture notes ; 42. |
| Subject: | |
| Format: | E-Resource Book |
| URL for this record: | http://pi.lib.uchicago.edu/1001/cat/bib/11096189 |
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| 100 | 1 | |a Clarke, Cathie J., |e author. |1 http://viaf.org/viaf/39695196 | |
| 245 | 1 | 0 | |a Dynamics of young star clusters and associations : |b Saas-Fee advanced course 42 / |c Cathie J. Clarke, Robert D. Mathieu and I. Neill Reid ; Swiss Society for Astrophysics and Astronomy. |
| 264 | 1 | |a Heidelberg : |b Springer, |c 2016. | |
| 264 | 4 | |c ©2016 | |
| 300 | |a 1 online resource. | ||
| 336 | |a text |b txt |2 rdacontent |0 http://id.loc.gov/vocabulary/contentTypes/txt | ||
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| 490 | 1 | |a Saas-fee advanced course ; |v 42 | |
| 588 | 0 | |a Online resource; title from PDF title page (EBSCO, viewed September 16, 2015). | |
| 504 | |a Includes bibliographical references. | ||
| 505 | 0 | |a Foreword; Preface; Contents; List of Figures; List of Tables; Part ITheory of Star Formation and DynamicalEvolution of Stellar Systems; 1 The Raw Material of Cluster Formation: Observational Constraints; 1.1 Overview of Molecular Cloud Observations; 1.2 Observational Techniques Applied to GMCs; 1.2.1 Molecular Line Emission; 1.2.2 Dust Emission; 1.2.3 Dust Absorption; 1.3 Magnetic Support and the Star Formation Efficiency Problem; 1.4 Scaling Relations; 1.5 GMCs and the Large-Scale ISM; 1.6 Summary: Key Observational Constraints for Simulations; References | |
| 505 | 8 | |a 2 The Numerical Tools for Star Cluster Formation Simulations2.1 The Pure Gravitational Problem; 2.2 Hydrodynamical Problems: A Quick Guide to SPH; 2.3 Adding `More Physics' to Hydrodynamical Codes; 2.4 Summary; References; 3 The Comparison of Observational and Simulation Data; 3.1 The Characterisation of Observational and Simulated Data; 3.1.1 Characterising Gaseous Structures; 3.1.2 Characterising Stellar Distributions; 3.1.3 Characterising the IMF; 3.2 Simulation Results: Bonnell et al. (2008) as a Case Study; 3.3 The Relationship Between Gas, Cores and Stars in Simulations | |
| 505 | 8 | |a 3.4 The Origin of the Stellar IMF in `Vanilla' Calculations3.5 Summary; References; 4 The Role of Feedback and Magnetic Fields; 4.1 Varying the Parameters; 4.2 Putting in More Physics; 4.2.1 Thermal Feedback; 4.2.2 Outflows; 4.2.3 Magnetic Fields; 4.2.4 Ionising Radiation; 4.3 Discussion; 4.4 Summary; References; 5 The Formation of Multiple Systems in Clusters; 5.1 The Formation of Multiple Stars in `Vanilla' Simulations; 5.1.1 Binary Star Statistics; 5.1.2 Disc Orientation in Protobinaries; 5.1.3 Predictions for Higher-Order Multiples | |
| 505 | 8 | |a 5.2 The Effect of `Additional Physics' on Multiple Star Formation5.3 Summary; References; 6 The Role of N-body Dynamics in Early Cluster Evolution; 6.1 Mass Segregation; 6.2 The Destruction of Binaries in Clusters; 6.3 Stellar Dynamics Plus Gas: Stellar Collisions; 6.4 Stellar Dynamics with Gas Removal: Infant Mortality; 6.5 Summary; References; 7 Concluding Issues; 7.1 Modelling Individual Clusters; 7.1.1 Gas-Free Studies; 7.1.2 Embedded Star-Forming Regions; 7.2 Imprint of Cluster Origin on Field Star Populations; 7.3 Imprint of Cluster Birthplace on Discs | |
| 505 | 8 | |a 7.4 The Birth Environment of the Sun7.5 Summary; References; Part IIKinematics of Star Clustersand Associations; 8 Introduction to Open Clusters; 8.1 Introduction; 8.2 Classical Open Clusters; 8.2.1 Definition; 8.2.2 Global Properties; 8.2.3 Internal Properties; 8.2.4 OB Associations; 8.3 Closing Thought; References; 9 Overview of Multiple Star Systems; 9.1 Introduction; 9.2 Field Solar-Type Binary Population; 9.3 Field OB Binary Population; 9.4 Open Cluster Solar-Type Binary Population; 9.5 Closing Thoughts; References; 10 Overview of Collisional Stellar Dynamics; 10.1 Introduction | |
| 650 | 0 | |a Stars |x Clusters. |0 http://id.loc.gov/authorities/subjects/sh85127422 | |
| 650 | 0 | |a Stars |x Formation. |0 http://id.loc.gov/authorities/subjects/sh85127431 | |
| 650 | 0 | |a Stars |x Evolution. | |
| 650 | 7 | |a SCIENCE / Astronomy |2 bisacsh | |
| 650 | 7 | |a Stars |x Clusters. |2 fast |0 (OCoLC)fst01131662 | |
| 650 | 7 | |a Stars |x Evolution. |2 fast |0 (OCoLC)fst01131672 | |
| 650 | 7 | |a Stars |x Formation. |2 fast |0 (OCoLC)fst01131674 | |
| 655 | 4 | |a Electronic books. | |
| 655 | 0 | |a Electronic books. | |
| 700 | 1 | |a Mathieu, Robert D., |e author. |1 http://viaf.org/viaf/24854403 | |
| 700 | 1 | |a Reid, I. Neill., |e author. |1 http://viaf.org/viaf/39685440 | |
| 710 | 2 | |a Schweizerische Gesellschaft für Astrophysik und Astronomie, |e issuing body. |0 http://id.loc.gov/authorities/names/n50054473 |1 http://viaf.org/viaf/148783599 | |
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| 830 | 0 | |a Saas-Fee advanced course ... lecture notes ; |v 42. | |
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