Skip to main content
  • Book
  • © 2015

Dynamics of the Milky Way

Tidal Streams and Extended Distribution Functions for the Galactic Disc

Authors:

  • 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)

Buy it now

Buying options

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

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

Table of contents (9 chapters)

  1. Front Matter

    Pages i-xxii
  2. Introduction

    • Jason Sanders
    Pages 1-17
  3. Stream-Orbit Misalignment

    • Jason Sanders
    Pages 109-134
  4. Stream Modelling in Angle-Frequency Space

    • Jason Sanders
    Pages 135-169
  5. Conclusions

    • Jason Sanders
    Pages 221-228
  6. Back Matter

    Pages 229-264

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

Buy it now

Buying options

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