國立虎尾科技大學 |

Dynamics of galaxies

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/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. -
電子資源:	https://doi.org/10.1017/CBO9780511731990
ISBN:	9780511731990

Dynamics of galaxies
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:

769071
Galaxies.

LC Class. No.: QB857 / .B47 2014

Dewey Class. No.: 523.112

Dynamics of galaxies
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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 769071
856 4 0 $u https://doi.org/10.1017/CBO9780511731990