Cargando…

Dynamics and Evolution of Galactic Nuclei.

Deep within galaxies like the Milky Way, astronomers have found a fascinating legacy of Einstein's general theory of relativity: supermassive black holes. Connected to the evolution of the galaxies that contain these black holes, galactic nuclei are the sites of uniquely energetic events, inclu...

Descripción completa

Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Merritt, David
Formato: Electrónico eBook
Idioma:Inglés
Publicado: New Jersey : Princeton University Press, 2013.
Colección:Princeton series in astrophysics.
Temas:
Acceso en línea:Texto completo
Tabla de Contenidos:
  • Cover
  • Title
  • Copyright
  • Dedication
  • Contents
  • Preface
  • Chapter 1 INTRODUCTION AND HISTORICAL OVERVIEW
  • Chapter 2 OBSERVATIONS OF GALACTIC NUCLEI AND SUPERMASSIVE BLACK HOLES
  • 2.1 Structure of galaxies and galactic nuclei
  • 2.2 Techniques for weighing black holes
  • 2.3 Supermassive black holes in the Local Group
  • 2.4 Phenomenology
  • 2.5 Evidence for intermediate-mass black holes
  • 2.6 Evidence for binary and multiple supermassive black holes
  • 2.7 Gravitational waves
  • Chapter 3 COLLISIONLESS EQUILIBRIA
  • 3.1 Orbits, integrals, and steady states
  • 3.2 Spherical nuclei
  • 3.3 The adiabatic growth model
  • 3.4 Axisymmetric nuclei
  • 3.5 Triaxial nuclei
  • Chapter 4 MOTION NEAR SUPERMASSIVE BLACK HOLES
  • 4.1 Keplerian orbits
  • 4.2 Perturbed orbits
  • 4.3 The post-Newtonian approximation
  • 4.4 Newtonian perturbations
  • 4.5 Relativistic orbits
  • 4.6 Capture
  • 4.7 Relativistic motion in the presence of a distributed mass
  • 4.8 Motion in the presence of a second massive body
  • 4.9 Stellar motions at the center of the Milky Way
  • Chapter 5 THEORY OF GRAVITATIONAL ENCOUNTERS
  • 5.1 Basic concepts and time of relaxation
  • 5.2 Diffusion coefficients
  • 5.3 Fokker-Planck equation
  • 5.4 Gravitational Brownian motion
  • 5.5 Orbit-averaged Fokker-Planck equation
  • 5.6 Gravitational encounters near a supermassive black hole
  • 5.7 Encounters with a spinning supermassive black hole
  • Chapter 6 LOSS-CONE DYNAMICS
  • 6.1 Spherical symmetry
  • 6.2 Nonspherical nuclei
  • 6.3 Binary and hypervelocity stars
  • 6.4 Relativistic loss cones and extreme-mass-ratio inspirals
  • Chapter 7 COLLISIONAL EVOLUTION OF NUCLEI
  • 7.1 Evolution of the stellar distribution around a supermassive black hole
  • 7.2 Cusp (re)generation
  • 7.3 Black-hole-driven expansion
  • 7.4 Massive perturbers
  • 7.5 Evolution of nuclei lacking massive black holes
  • Chapter 8 BINARY AND MULTIPLE SUPERMASSIVE BLACK HOLES
  • 8.1 Interaction of a massive binary with field stars
  • 8.2 Massive binary at the center of a galaxy: I. Early evolution
  • 8.3 Massive binary at the center of a galaxy: II. Late evolution
  • 8.4 Interaction of binary supermassive black holes with gas
  • 8.5 Simulations of galaxy mergers
  • 8.6 Dynamics of intermediate-mass black holes
  • 8.7 Triple supermassive black holes and the final-parsec problem
  • Suggestions for Further Reading
  • References
  • Index