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Origin of the Galaxy and Local Group: Saas-Fee Advanced Course 37 Swiss Society for Astrophysics and Astronomy 2014 ed. [Hardback]

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  • Formāts: Hardback, 231 pages, height x width: 235x155 mm, weight: 4912 g, 70 Illustrations, color; 36 Illustrations, black and white; IX, 231 p. 106 illus., 70 illus. in color., 1 Hardback
  • Sērija : Saas-Fee Advanced Course 37
  • Izdošanas datums: 19-Feb-2014
  • Izdevniecība: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3642417191
  • ISBN-13: 9783642417191
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Origin of the Galaxy and Local Group: Saas-Fee Advanced Course 37 Swiss Society for Astrophysics and Astronomy 2014 ed.Palielināt
  • Formāts: Hardback, 231 pages, height x width: 235x155 mm, weight: 4912 g, 70 Illustrations, color; 36 Illustrations, black and white; IX, 231 p. 106 illus., 70 illus. in color., 1 Hardback
  • Sērija : Saas-Fee Advanced Course 37
  • Izdošanas datums: 19-Feb-2014
  • Izdevniecība: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3642417191
  • ISBN-13: 9783642417191
Citas grāmatas par šo tēmu:
Permanent link: https://www.kriso.lv/db/9783642417191.html
Keywords:
Presenting updated and elaborated lecture notes of the 37th Saas-Fee Advanced Course organised by the Swiss Society for Astrophysics and Astronomy, this book explores of one of the hottest research topics in astrophysics: how our Milky Way galaxy formed.

This volume contains the updated and expanded lecture notes of the 37th Saas-Fee Advanced Course organised by the Swiss Society for Astrophysics and Astronomy. It offers the most comprehensive and up to date review of one of the hottest research topics in astrophysics - how our Milky Way galaxy formed. Joss Bland-Hawthorn & Ken Freeman lectured on Near Field Cosmology - The Origin of the Galaxy and the Local Group. Francesca Matteucci’s chapter is on Chemical evolution of the Milky Way and its Satellites. As designed by the SSAA, books in this series – and this one too – are targeted at graduate and PhD students and young researchers in astronomy, astrophysics and cosmology. Lecturers and researchers entering the field will also benefit from the book.
1 Near Field Cosmology: The Origin of the Galaxy and the Local Group
1(144)
Joss Bland-Hawthorn
Kenneth Freeman
1.1 Prologue
1(1)
1.2 Far Field Cosmology
2(14)
1.2.1 The Cosmic Microwave Background
4(3)
1.2.2 The First Stars
7(3)
1.2.3 The First Black Holes
10(2)
1.2.4 The First Dark Haloes
12(3)
1.2.5 Reionization and the First Galaxies
15(1)
1.3 Lessons from Galaxy Redshift Surveys
16(11)
1.3.1 Evolution and Environment
19(1)
1.3.2 Accretion and Feedback
20(2)
1.3.3 Baryon Inventory and Metal Enrichment
22(3)
1.3.4 Chemical Evolution in Galaxies
25(1)
1.3.5 Milky Way and Local Group Analogues in the Real Universe
25(1)
1.3.6 Milky Way and Local Group Analogues in Simulated Universes
26(1)
1.4 Gas Accretion onto Galaxies
27(18)
1.4.1 Introduction
27(1)
1.4.2 Earliest Epoch of Gas Accretion
28(2)
1.4.3 Early Ideas on Galaxy Accretion
30(2)
1.4.4 Accretion Shocks
32(2)
1.4.5 Cooling Flows
34(1)
1.4.6 Cold Flows
35(3)
1.4.7 Warm Flows
38(1)
1.4.8 Accretion via Major and Minor Mergers
38(1)
1.4.9 Accretion of High Velocity Clouds
39(6)
1.5 Near Field Cosmology
45(10)
1.5.1 Introduction
45(2)
1.5.2 A Working Model of How the Galaxy Formed
47(2)
1.5.3 Timescales and Fossils
49(2)
1.5.4 Stellar Age Dating
51(3)
1.5.5 Goals of Near Field Cosmology
54(1)
1.6 Structure of the Galaxy
55(8)
1.6.1 The Bulge
55(4)
1.6.2 The Disk
59(1)
1.6.3 The Stellar Halo
60(2)
1.6.4 The Dark Halo
62(1)
1.7 Signatures of Galaxy Formation
63(23)
1.7.1 Zero Order Signatures: Information Preserved Since Dark Matter Virialized
63(5)
1.7.2 First Order Signatures: Information Preserved Since the Main Epoch of Baryon Dissipation
68(6)
1.7.3 Second Order Signatures: Major Processes Involved in Subsequent Evolution
74(12)
1.8 Reconstructing the Past Through Chemical Tagging
86(18)
1.8.1 Unravelling a Dissipative Process
86(2)
1.8.2 How Many Star Clusters?
88(1)
1.8.3 Cluster Chemistry
89(1)
1.8.4 Chemical Homogeneity
90(2)
1.8.5 Unique Chemical Signatures
92(1)
1.8.6 Primary Requirements of Chemical Tagging
92(5)
1.8.7 Candidates for Chemical Tagging
97(3)
1.8.8 Short-Term Goal: Size and Structure in a Multi-Dimensional C-Space
100(1)
1.8.9 Long-Term Goal: Reconstructing Ancient Star Groups from Unique Chemical Signatures
101(3)
1.9 Epilogue: Challenges for the Future
104(8)
1.9.1 The Limitations of Near Field Cosmology: Are We Really Putting ˆCDM to the Test?
104(2)
1.9.2 Future Surveys
106(3)
Appendix A The Discovery of Dark Matter in Galaxies
109(3)
Appendix B Stellar Data: Sources and Techniques
112(1)
B.1 Data Needed for Galactic Archaeology
112(6)
B.2 Sources of Data
118(7)
B.3 Sources of Models
125(20)
References
128(17)
2 Chemical Evolution of the Milky Way and Its Satellites
145(84)
Francesca Matteucci
2.1 How to Model Galactic Chemical Evolution
145(13)
2.1.1 The Initial Conditions
146(1)
2.1.2 Birthrate Function
146(4)
2.1.3 Stellar Yields
150(8)
2.1.4 Gas Flows
158(1)
2.2 Basic Equations for Chemical Evolution
158(6)
2.2.1 Yields per Stellar Generation
158(1)
2.2.2 Analytical Models
159(3)
2.2.3 Detailed Numerical Models
162(2)
2.3 The Milky Way
164(30)
2.3.1 The Formation of the Milky Way
164(2)
2.3.2 The Two-Infall Model
166(1)
2.3.3 Detailed Recipes for the Two-Infall Model
167(3)
2.3.4 The Chemical Enrichment History of the Solar Vicinity
170(11)
2.3.5 The Galactic Disk
181(5)
2.3.6 The Galactic Bulge
186(8)
2.4 What We Have Learned About the Milky Way
194(1)
2.5 The Time-Delay Model and the Hubble Sequence
194(4)
2.5.1 Star Formation and Hubble Sequence
195(3)
2.6 Dwarf Spheroidals of the Local Group
198(14)
2.6.1 How do dSphs Form?
198(2)
2.6.2 Observations of dSphs
200(1)
2.6.3 Chemical Evolution of dSphs
200(8)
2.6.4 What Have we Learned About dSphs?
208(4)
2.7 Ultra-Faint Dwarfs in the Local Group
212(2)
2.8 Other Spirals
214(3)
2.8.1 Chemical Models for External Spirals
215(2)
2.9 Cosmic Chemical Evolution
217(12)
References
222(7)
Index 229
Joss Bland-Hawthorn holds the Federation Fellow Professorship at the Institute of Astronomy, School of Physics, University of Sydney. He is doing research on near-field and far-field cosmology and is also working in instrument science. Kenneth Charles Freeman is Duffield Professor of Astronomy in the Research School of Astronomy and Astrophysics at the Mount Stromlo Observatory of the Australian National University in Canberra. His research interests are in the formation and dynamics of galaxies and globular clusters. He received several international awards. Francesca Matteucci is associate professor at the University of Trieste, Italy, where she teaches Stellar Physics. Her field of research is the chemical evolution of galaxies of different morphological type, supernova rates and supernova progenitors.