Skip to main content

Dynamics of the Milky Way

Tidal Streams and Extended Distribution Functions for the Galactic Disc

  • Book
  • © 2015

Overview

  • Nominated as an outstanding Ph.D. thesis by the University of Oxford, UK
  • Presents an introduction to dynamical modelling of the Milky Way
  • Discusses new methods for the efficient approximation of angle-action variables
  • Introduces new action-based models for tidal streams and chemo dynamical models for the Galactic disc
  • Includes supplementary material: sn.pub/extras

Part of the book series: Springer Theses (Springer Theses)

This is a preview of subscription content, log in via an institution to check access.

Access this book

eBook USD 84.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Hardcover Book USD 109.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access

Licence this eBook for your library

Institutional subscriptions

Table of contents (9 chapters)

Keywords

About this book

This work presents a study of methods useful for modeling and understanding dynamical systems in the Galaxy. A natural coordinate system for the study of dynamical systems is the angle-action coordinate system. New methods for the approximation of the action-angle variables in general potentials are presented and discussed. These new tools are applied to the construction of dynamical models for two of the Galaxy’s components: tidal streams and the Galactic disc. Tidal streams are remnants of tidally stripped satellites in the Milky Way that experience the effects of the large scale structure of the Galactic gravitational potential, while the Galactic disc provides insights into the nature of the Galaxy near the Sun. Appropriate action-based models are presented and discussed for these components, and extended to include further information such as the metallicity of stars.

Authors and Affiliations

  • Institute for Astronomy, University of Cambridge, Cambridge, United Kingdom

    Jason Sanders

Bibliographic Information

Publish with us