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Not-so-simple stellar populations in star clusters

Author: Chengyuan Li
Publisher: Singapore : Springer, [2017] ©2017
Series: Springer theses.
Edition/Format:   eBook : Document : EnglishView all editions and formats
Summary:
This book focuses on understanding the stellar populations of massive star clusters, which aims to investigate the origin, evolution and properties of binary systems, their collision products, as well as the general characteristics (e.g. ages, metal content) of stellar population(s) in star clusters. It introduces the basic background knowledge of various stellar populations in star clusters as well as their  Read more...
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Genre/Form: Electronic books
Additional Physical Format: Print version:
Li, Chengyuan.
Not-so-simple stellar populations in star clusters.
Singapore : Springer, [2017]
(OCoLC)991690447
Material Type: Document, Internet resource
Document Type: Internet Resource, Computer File
All Authors / Contributors: Chengyuan Li
ISBN: 9789811056819 9811056811
OCLC Number: 1004720863
Notes: "Doctoral thesis accepted by the Department of Astronomy at Peking University, Beijing, China."
Description: 1 online resource.
Contents: Supervisor's Foreword; Preface; Scope; Content; Audience; Acknowledgements; Contents; Acronyms; Part I Star Formation, Evolution and Stellar Populations in Star Clusters; 1 Stellar Evolution and Populations; 1.1 The Early History of Researches on Star Clusters; 1.2 A Simple Introduction on Stellar Evolution; 1.2.1 The Main Sequence; 1.2.2 The Turn-Off and Sub-giant Stage; 1.2.3 The Red-Giant Stage; 1.2.4 Stellar Age Versus Its Initial Mass; 1.3 Simple Stellar Populations; 1.3.1 Describing the Simple Stellar Population; 1.4 Not-So-Simple Stellar Populations: Multiple Stellar Populations. 1.4.1 Describing the Multiple Stellar Populations2 Researches of Stellar Populations in Star Clusters; 2.1 Stellar Populations: We Think We Know Until Everything Change; 2.1.1 Why Most Clusters Should be Simple Stellar Populations?; 2.1.2 Complicated Stellar Populations in Star Clusters; 2.2 Proposed Scenarios; 2.2.1 The Extended Main Sequence Turn-Off Regions in Star Clusters; 2.2.2 Multiple Stellar Populations in Old Globular Clusters; Part II Researches on Stellar Populations in Massive Star Clusters; 3 Binary Fraction in Young Massive Star Clusters; 3.1 Introduction; 3.2 Data Reduction. 5.2 Data Reduction and Analysis5.3 Main Results; 5.3.1 Sub-giant Branch Stars; 5.3.2 Red-Giant Branch Stars; 5.4 Physical Inplications; 5.5 Conclusion; 6 Do Intermediate-Age Star Clusters Have Extended Star Formation Histories?; 6.1 Introduction; 6.2 Data Reduction; 6.3 Main Results; 6.3.1 NGC1651; 6.3.2 NGC411; 6.3.3 NGC419; 6.4 Physical Discussion; 6.5 Conclusion; Part III Not-So-Simple Stellar Populations in Massive Star Clusters, Where Do We Stand?; 7 Lessons Learned from This Thesis; 7.1 Do the Young Massive Clusters Harbor Multiple Stellar Populations? 7.2 No Evidence of Multiple Stellar Populations in Intermediate-Age Star Clusters7.3 Do Globular Clusters have Another Origin?; 7.4 Epilogue; References.
Series Title: Springer theses.
Responsibility: Chengyuan Li.

Abstract:

This book focuses on understanding the stellar populations of massive star clusters and aims to investigate the origin, evolution and properties of binary systems, their collision products, as well  Read more...

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