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Mass is one of the most fundamental quantities that characterise stellar systems, from star clusters to large galaxies. It determines both the internal dynamics of the system and its gravitational interaction with other systems. For the galaxies in the Local Group, a real revolution in the topic has occurred with the Gaia satellite that provides six-dimensional data (three-dimensional positions and velocities) for almost 1.5 billion sources, located both in the Milky Way and in Local Group galaxies. IAU Symposium 379 gathered together the community working on this topic to discuss and collect recent advances and provide an opportunity for researchers to meet, exchange ideas, and compare methods and hypothesis. Measuring galaxy masses at different scales in the Local Group impacts a broad range of astronomy, from stars and star clusters, to the Milky Way, distant galaxies, and cosmology.
Edited by:   , , , , , , , ,
Imprint:   Cambridge University Press
Country of Publication:   United Kingdom
ISBN:   9781009399111
ISBN 10:   100939911X
Series:   Proceedings of the International Astronomical Union Symposia and Colloquia
Pages:   400
Publication Date:  
Audience:   General/trade ,  ELT Advanced
Format:   Hardback
Publisher's Status:   Forthcoming
Part I. From Ground and Space; Part II. Sizes, Masses and Formation Histories of the Milky Way and Andromeda; Part III. Dwarf Galaxies; Part IV. The Magellanic System; Part V. Near-field Cosmology and Galaxy Masses Beyond the Local Group.

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