Rediscovering Our Galaxy (IAU S334)

Author:   Cristina Chiappini ,  Ivan Minchev ,  Else Starkenburg ,  Marica Valentini
Publisher:   Cambridge University Press
ISBN:  

9781107192348


Pages:   500
Publication Date:   13 September 2018
Format:   Hardback
Availability:   Available To Order   Availability explained
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Rediscovering Our Galaxy (IAU S334)


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Overview

Astronomers are at a crucial point in our understanding of the Milky Way. Deciphering the assembly history of our galaxy requires detailed mapping of the structure, dynamics, chemical composition, and age distribution of its stellar populations. In the last decade, astrometric, spectroscopic, photometric, and asteroseismic surveys have started to unveil the inner- and outermost regions of the Milky Way. IAU Symposium 334 explores the still open questions and focusses on the concepts emerging from the analysis of these large, new, and complex datasets. This volume presents a summary of these topics, including the current novel data and the challenges they already pose to modeling, before Gaia end-of-mission, PLATO, and large spectroscopic surveys such as WEAVE and 4MOST are about to start. Graduate students and researchers will learn that, in this golden era of galactic archaeology, we are about to rediscover our galaxy.

Full Product Details

Author:   Cristina Chiappini ,  Ivan Minchev ,  Else Starkenburg ,  Marica Valentini
Publisher:   Cambridge University Press
Imprint:   Cambridge University Press
Dimensions:   Width: 18.00cm , Height: 2.30cm , Length: 25.70cm
Weight:   0.820kg
ISBN:  

9781107192348


ISBN 10:   110719234
Pages:   500
Publication Date:   13 September 2018
Audience:   Professional and scholarly ,  College/higher education ,  Professional & Vocational ,  Postgraduate, Research & Scholarly
Format:   Hardback
Publisher's Status:   Active
Availability:   Available To Order   Availability explained
We have confirmation that this item is in stock with the supplier. It will be ordered in for you and dispatched immediately.

Table of Contents

1. Tracers of the oldest Milky Way fossil records and Halo Assembly; 2. Disentangling mixed populations in the central regions of the Milky Way; 3. Galactic disks – chemodynamical properties and models; 4. Towards ages: Gaia DR1, asteroseismology, and precise abundances; 5. Stellar evolution models and stellar yields; 6. Milky Way potential and disk dynamics; 7. Cosmological simulations of Milky-Way-like galaxies; 8. Challenges in data and modeling; 9. Future outlook.

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