大葉大學圖書館 |

Dynamics of galaxies[electronic resource] /

紀錄類型:	書目-電子資源 : Monograph/item
杜威分類號:	523.112
書名/作者:	Dynamics of galaxies/ Giuseppe Bertin.
作者:	Bertin, Giuseppe.
出版者:	Cambridge : : Cambridge University Press,, 2014.
面頁冊數:	xvi, 468 p. : : ill., digital ;; 24 cm.
標題:	Galaxies.
ISBN:	9780511731990
ISBN:	9781107000544
摘要、提要註:	Our understanding of galaxies, the building blocks of the Universe has advanced significantly in recent years. New observations from ground- and space-based telescopes, the discovery of dark matter, and new insights into its distribution have been instrumental in this. This textbook provides graduate students with a modern introduction to the gravitationally determined structure and evolution of galaxies. Readers will also benefit from detailed discussions of the issues involved in the process of modeling complex stellar systems. Additionally, the text provides an accessible framework for interpreting observations and devising new observational tests. Based on the author's extensive teaching experience, this second edition features an up-to-date view of basic phenomenology, a discussion of the structure of dark halos in galaxies, the dynamics of quasi-relaxed stellar systems and globular clusters, galaxies and gravitational lensing and an introduction to self-gravitating accretion disks. Extended problem sets are available from the accompanying resources website: www.cambridge.org/9781107000544.
電子資源:	https://doi.org/10.1017/CBO9780511731990

Dynamics of galaxies[electronic resource] /
Bertin, Giuseppe.

Dynamics of galaxies[electronic resource] /Giuseppe Bertin. - Second edition. - Cambridge :Cambridge University Press,2014. - xvi, 468 p. :ill., digital ;24 cm.

Basic phenomenology --

Our understanding of galaxies, the building blocks of the Universe has advanced significantly in recent years. New observations from ground- and space-based telescopes, the discovery of dark matter, and new insights into its distribution have been instrumental in this. This textbook provides graduate students with a modern introduction to the gravitationally determined structure and evolution of galaxies. Readers will also benefit from detailed discussions of the issues involved in the process of modeling complex stellar systems. Additionally, the text provides an accessible framework for interpreting observations and devising new observational tests. Based on the author's extensive teaching experience, this second edition features an up-to-date view of basic phenomenology, a discussion of the structure of dark halos in galaxies, the dynamics of quasi-relaxed stellar systems and globular clusters, galaxies and gravitational lensing and an introduction to self-gravitating accretion disks. Extended problem sets are available from the accompanying resources website: www.cambridge.org/9781107000544.

ISBN: 9780511731990Subjects--Topical Terms:

465118
Galaxies.

LC Class. No.: QB857 / .B47 2014

Dewey Class. No.: 523.112

Dynamics of galaxies[electronic resource] /
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505 0 $t Basic phenomenology -- $t Scales -- $t Observational windows -- $t Classifications -- $t Photometry, kinematics, and dark matter -- $t Basic questions, semiempirical approach, and the dynamical window -- $t Physical models -- $t Self-gravity and relation to plasma physics -- $t Relaxation times, absense of thermodynamical equilibrium -- $t Models -- $t Equilibrium and stability : symmetry and symmetry breaking -- $t Classical ellipsoids -- $t Introduction to dispersive waves -- $t Jeans instability -- $t Spiral galaxies -- $t Orbits -- $t The basic state : vertical and horizontal equilibrium of the disk -- $t Density waves -- $t Roles of gas -- $t Global spiral modes -- $t Spiral structure in galaxies -- $t Bending waves -- $t Dark matter in spiral galaxies -- $t Elliptical galaxies -- $t Orbits -- $t Stellar dynamical models -- $t Stability -- $t Dark matter in elliptical galaxies -- $t In perspective -- $t Selected aspects of formation and evolution -- $t Galaxies and gravitational lensing -- $t Self-gravitating accretion disks.
520 $a Our understanding of galaxies, the building blocks of the Universe has advanced significantly in recent years. New observations from ground- and space-based telescopes, the discovery of dark matter, and new insights into its distribution have been instrumental in this. This textbook provides graduate students with a modern introduction to the gravitationally determined structure and evolution of galaxies. Readers will also benefit from detailed discussions of the issues involved in the process of modeling complex stellar systems. Additionally, the text provides an accessible framework for interpreting observations and devising new observational tests. Based on the author's extensive teaching experience, this second edition features an up-to-date view of basic phenomenology, a discussion of the structure of dark halos in galaxies, the dynamics of quasi-relaxed stellar systems and globular clusters, galaxies and gravitational lensing and an introduction to self-gravitating accretion disks. Extended problem sets are available from the accompanying resources website: www.cambridge.org/9781107000544.
650 0 $a Galaxies. $3 465118
856 4 0 $u https://doi.org/10.1017/CBO9780511731990