Local Group Cosmology

doi:10.1017/CBO9781139152303

One of the most fascinating unresolved problems of modern astrophysics is how the galaxies we observe today were formed. The Lambda-Cold Dark Matter paradigm predicts that large spiral galaxies such as the Milky Way formed through accretion and tidal disruption of satellite galaxies. The galaxies of the Local Group provide the best laboratory in which to investigate these galaxy formation processes because they can be studied with sufficiently high resolution to exhume fossils of galactic evolution embedded in the spatial distribution, kinematics, and chemical abundances of their oldest stars. Based on the twentieth Winter School of the Canary Islands Institute of Astrophysics, this volume provides a firm grounding for graduate students and early career researchers working on Local Group cosmology. It presents modules from eight eminent and experienced scientists at the forefront of Local Group research, and includes overviews of observational techniques, diagnostic tools, and various theoretical models.

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Local Group Cosmology

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Frontmatter
pp i-vi

Contents
pp vii-viii

List of contributors
pp ix-x

List of participants
pp xi-xii

Preface
pp xiii-xiv

Acknowledgments
pp xv-xvi

Abbreviations
pp xvii-xviii

1 - The formation of the Milky Way in the CDM paradigm
pp 1-46

2 - Dark matter content and tidal effects in Local Group dwarf galaxies
pp 47-94

3 - Notes on the missing satellites problem
pp 95-122

4 - The Milky Way satellite galaxies as critical tests of contemporary cosmological theory
pp 123-161

5 - Stellar tidal streams
pp 162-191

6 - Tutorial: The analysis of colour-magnitude diagrams
pp 192-225

7 - Tutorial: Modeling tidal streams using N-body simulations
pp 226-232

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