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Dynamics of the Milky Waytidal strea...
~
Milky Way.
Dynamics of the Milky Waytidal streams and extended distribution functions for the galactic disc /
Record Type:
Electronic resources : Monograph/item
Title/Author:
Dynamics of the Milky Wayby Jason Sanders.
Reminder of title:
tidal streams and extended distribution functions for the galactic disc /
Author:
Sanders, Jason.
Published:
Cham :Springer International Publishing :2015.
Description:
xxii, 264 p. :ill., digital ;24 cm.
Contained By:
Springer eBooks
Subject:
Galactic dynamics.
Subject:
Milky Way.
Online resource:
http://dx.doi.org/10.1007/978-3-319-18772-3
ISBN:
9783319187723 (electronic bk.)
Dynamics of the Milky Waytidal streams and extended distribution functions for the galactic disc /
Sanders, Jason.
Dynamics of the Milky Way
tidal streams and extended distribution functions for the galactic disc /[electronic resource] :by Jason Sanders. - Cham :Springer International Publishing :2015. - xxii, 264 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Introduction -- Angle-Action Estimation in a General Axisymmetric Potential -- Actions, Angles and Frequencies from Numerically Integrated Orbits -- Action Estimation Using a Triaxial Stackel Approximation -- Stream-Orbit Misalignment -- Stream Modelling in Angle-Frequency Space -- Determining the Velocity Dispersion of the Thick Disc -- Extended Distribution Functions for the Galactic Disc -- Conclusions.
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.
ISBN: 9783319187723 (electronic bk.)
Standard No.: 10.1007/978-3-319-18772-3doiSubjects--Topical Terms:
727030
Galactic dynamics.
Subjects--Geographical Terms:
560752
Milky Way.
LC Class. No.: QB857.7
Dewey Class. No.: 523.113
Dynamics of the Milky Waytidal streams and extended distribution functions for the galactic disc /
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tidal streams and extended distribution functions for the galactic disc /
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Introduction -- Angle-Action Estimation in a General Axisymmetric Potential -- Actions, Angles and Frequencies from Numerically Integrated Orbits -- Action Estimation Using a Triaxial Stackel Approximation -- Stream-Orbit Misalignment -- Stream Modelling in Angle-Frequency Space -- Determining the Velocity Dispersion of the Thick Disc -- Extended Distribution Functions for the Galactic Disc -- Conclusions.
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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.
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Physics and Astronomy (Springer-11651)
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EB QB857.7 S215 2015
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http://dx.doi.org/10.1007/978-3-319-18772-3
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