did-you-know? rent-now

Amazon no longer offers textbook rentals. We do!

did-you-know? rent-now

Amazon no longer offers textbook rentals. We do!

We're the #1 textbook rental company. Let us show you why.

9780691130262

Galactic Dynamics

by
  • ISBN13:

    9780691130262

  • ISBN10:

    0691130264

  • Edition: 2nd
  • Format: Hardcover
  • Copyright: 2008-01-07
  • Publisher: Princeton Univ Pr
  • Purchase Benefits
  • Free Shipping Icon Free Shipping On Orders Over $35!
    Your order must be $35 or more to qualify for free economy shipping. Bulk sales, PO's, Marketplace items, eBooks and apparel do not qualify for this offer.
  • eCampus.com Logo Get Rewarded for Ordering Your Textbooks! Enroll Now
List Price: $120.00 Save up to $58.14
  • Digital
    $61.86
    Add to Cart

    DURATION
    PRICE

Supplemental Materials

What is included with this book?

Summary

Since it was first published in 1987,Galactic Dynamicshas become the most widely used advanced textbook on the structure and dynamics of galaxies and one of the most cited references in astrophysics. Now, in this extensively revised and updated edition, James Binney and Scott Tremaine describe the dramatic recent advances in this subject, makingGalactic Dynamicsthe most authoritative introduction to galactic astrophysics available to advanced undergraduate students, graduate students, and researchers. Every part of the book has been thoroughly overhauled, and many sections have been completely rewritten. Many new topics are covered, including N-body simulation methods, black holes in stellar systems, linear stability and response theory, and galaxy formation in the cosmological context. Binney and Tremaine, two of the world's leading astrophysicists, use the tools of theoretical physics to describe how galaxies and other stellar systems work, succinctly and lucidly explaining theoretical principles and their applications to observational phenomena. They provide readers with an understanding of stellar dynamics at the level needed to reach the frontiers of the subject. This new edition of the classic text is the definitive introduction to the field.

Author Biography

James Binney is professor of physics at the University of Oxford. His books include "Galactic Astronomy". Scott Tremaine is the Richard Black Professor of Astrophysics at the Institute for Advanced Study and a member of the National Academy of Sciences. Both are fellows of the Royal Society.

Table of Contents

Prefacep. xiii
Introductionp. 1
An overview of the observationsp. 5
Collisionless systems and the relaxation timep. 33
The relaxation timep. 34
The cosmological contextp. 37
Potential Theoryp. 55
General resultsp. 56
The potential-energy tensorp. 59
Spherical systemsp. 60
Potential-density pairs for attened systemsp. 72
Multipole expansionp. 78
The potentials of spheroidal and ellipsoidal systemsp. 83
The potentials of disksp. 96
The potential of our Galaxyp. 110
Potentials from functional expansionsp. 118
Poisson solvers for N-body codesp. 122
The Orbits of Starsp. 142
Orbits in static spherical potentialsp. 143
Orbits in axisymmetric potentialsp. 159
Orbits in planar non-axisymmetric potentialsp. 171
Numerical orbit integrationp. 196
Angle-action variablesp. 211
Slowly varying potentialsp. 237
Perturbations and chaosp. 243
Orbits in elliptical galaxiesp. 262
Equilibria of Collisionless Systemsp. 274
The collisionless Boltzmann equationp. 275
Jeans theoremsp. 283
DFs for spherical systemsp. 287
DFs for axisymmetric density distributionsp. 312
DFs for razor-thin disksp. 329
Using actions as arguments of the DFp. 333
Particle-based and orbit-based modelsp. 338
The Jeans and virial equationsp. 347
Stellar kinematics as a mass detectorp. 365
The choice of equilibriump. 376
Stability of Collisionless Systemsp. 394
Introductionp. 394
The response of homogeneous systemsp. 401
General theory of the response of stellar systemsp. 417
The energy principle and secular stabilityp. 423
The response of spherical systemsp. 432
The stability of uniformly rotating systemsp. 439
Disk Dynamics and Spiral Structurep. 456
Fundamentals of spiral structurep. 458
Wave mechanics of differentially rotating disksp. 481
Global stability of differentially rotating disksp. 505
Damping and excitation of spiral structurep. 518
Barsp. 528
Warping and buckling of disksp. 539
Kinetic Theoryp. 554
Relaxation processesp. 555
General resultsp. 559
The thermodynamics of self-gravitating systemsp. 567
The Fokker Planck approximationp. 573
The evolution of spherical stellar systemsp. 596
Summaryp. 633
Collisions and Encounters of Stellar Systemsp. 639
Dynamical frictionp. 643
High-speed encountersp. 655
Tidesp. 674
Encounters in stellar disksp. 685
Mergersp. 695
Galaxy Formationp. 716
Linear structure formationp. 717
Nonlinear structure formationp. 733
N-body simulations of clusteringp. 751
Star formation and feedbackp. 760
Conclusionsp. 765
Useful numbersp. 770
Mathematical backgroundp. 771
Special functionsp. 785
Mechanicsp. 792
Delaunay variables for Kepler orbitsp. 805
Fluid mechanicsp. 807
Discrete Fourier transformsp. 818
The Antonov Lebovitz theoremp. 822
The Doremus Feix Baumann theoremp. 823
Angular-momentum transport in disksp. 825
Derivation of the reduction factorp. 830
The diffusion coefficientsp. 833
The distribution of binary energiesp. 838
Referencesp. 842
Indexp. 857
Table of Contents provided by Publisher. All Rights Reserved.

Supplemental Materials

What is included with this book?

The New copy of this book will include any supplemental materials advertised. Please check the title of the book to determine if it should include any access cards, study guides, lab manuals, CDs, etc.

The Used, Rental and eBook copies of this book are not guaranteed to include any supplemental materials. Typically, only the book itself is included. This is true even if the title states it includes any access cards, study guides, lab manuals, CDs, etc.

Rewards Program