Fundamentals of galaxy dynamics, formation and evolution

Ignacio Ferreras presents a concise introduction to extragalactic astrophysics, with emphasis on stellar dynamics, and the growth of density fluctuations in an expanding Universe. Additional chapters are devoted to smaller systems (stellar clusters) and larger ones (galaxy clusters)

Bibliographic Details
Main Author: Ferreras, Ignacio
Format: eBook
Language:English
Published: London UCL Press 2019, 2019
Subjects:
Online Access:
Collection: JSTOR Open Access Books - Collection details see MPG.ReNa
LEADER 03917nam a2200469 u 4500
001 EB001866803
003 EBX01000000000000001030883
005 00000000000000.0
007 tu|||||||||||||||||||||
008 190506 r ||| eng
020 |a 1911307649 
020 |z 1911307622 
020 |a 1911307622 
020 |z 9781911307624 
020 |a 9781911307624 
020 |z 1911307630 
020 |a 1911307630 
020 |z 9781911307631 
020 |a 9781911307631 
020 |a 9781911307648 
050 4 |a QB810 
100 1 |a Ferreras, Ignacio 
245 0 0 |a Fundamentals of galaxy dynamics, formation and evolution  |h Elektronische Ressource  |c Ignacio Ferreras 
260 |a London  |b UCL Press  |c 2019, 2019 
300 |a 1 volume  |b illustrations (black and white) 
505 0 |a Includes bibliographical references and index 
505 0 |a 4.6. The potential of the Galaxy5. Specific aspects of disc and elliptical galaxies; 5.1. 'Hot' versus 'Cold' dynamical systems; 5.2. Scaling relations; 5.3. Rotation versus 'pressure' in early-type galaxies; 5.4. A brief introduction to spiral arms in disc galaxies; 6. Galactic chemical enrichment; 6.1. Nucleosynthesis and the formation of galaxies; 6.2. General aspects of galactic chemical enrichment; 6.3. Basic equations of galactic chemical enrichment; 6.4. Chemistry as a cosmic clock; 7. The growth of density fluctuations; 7.1. A cosmology primer; 7.2. Linear regime 
505 0 |a 3.2. The distribution function3.3. Relaxation time; 3.4. Local and distant encounters; 3.5. Collisionless Boltzmann equation; 3.6. Isolating integrals: Jeans theorem; 3.7. Examples of distribution functions; 3.8. Jeans equations; 3.9. The virial theorem; 3.10. Beyond the collisionless Boltzmann equation: The Fokker-Planck equation; 4. Understanding our Galaxy; 4.1. General description of the Galaxy; 4.2. Differential rotation in the Galaxy; 4.3. Vertical motion; 4.4. The collisionless Boltzmann equation in galactic coordinates; 4.5. Application of Jeans equations 
505 0 |a Intro; Title Page; Copyright; Contents; List of figures; List of tables; Preface; Acknowledgements; 1. An introduction to galaxy formation; 1.1. The main ingredients of a galaxy; 1.2. Observables; 1.3. Physical processes; 1.4. Stellar clusters; 1.5. A technical note on astronomical observations; 2. The classical theory of gravitation; 2.1. Gravitational force; 2.2. The Kepler problem; 2.3. Potential theory; 2.4. Gravitational potential energy; 2.5. Potential/density pairs: A few fundamental cases; 2.6. Two-dimensional projection; 3. A statistical treatment of stellar systems; 3.1. Phase space 
505 0 |a 7.3. Spherical collapse7.4. Press-Schechter formalism; 7.5. Correlation function; 7.6. Cooling and the masses of galaxies; 8. Smaller stellar systems: Stellar clusters; 8.1. Open and globular clusters; 8.2. Internal evolutionary effects; 8.3. External effects: Tidal disruption; 8.4. Cluster evaporation: King models; 9. Larger stellar systems: Galaxy clusters; 9.1. The most massive structures; 9.2. X-ray measurements of the cluster mass; 9.3. Gravitational lensing; 9.4. Clusters and cosmology; 9.5. Environment-related processes; Further reading; Index 
653 |a Astrophysics 
653 |a Galaxies / Formation 
653 |a Stellar dynamics 
653 |a SCIENCE / Astronomy 
653 |a Galaxies / Evolution 
041 0 7 |a eng  |2 ISO 639-2 
989 |b ZDB-39-JOA  |a JSTOR Open Access Books 
776 |z 1911307614 
776 |z 9781911307617 
856 4 0 |u https://www.jstor.org/stable/10.2307/j.ctv8jnzhq  |x Verlag  |3 Volltext 
082 0 |a 523.83 
520 |a Ignacio Ferreras presents a concise introduction to extragalactic astrophysics, with emphasis on stellar dynamics, and the growth of density fluctuations in an expanding Universe. Additional chapters are devoted to smaller systems (stellar clusters) and larger ones (galaxy clusters)