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.

9780226144153

The Physics of Extragalactic Radio Sources

by
  • ISBN13:

    9780226144153

  • ISBN10:

    0226144151

  • Format: Hardcover
  • Copyright: 2002-01-01
  • Publisher: Univ of Chicago 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: $72.00

Summary

Extragalactic radio sources are among the most unusual and spectacular objects in the universe, with sizes in excess of millions of light years, radiated energies over ten times those of normal galaxies, and a unique morphology. They reveal some of the most dramatic physical events ever seen and provide essential clues to the basic evolutionary tracks followed by all galaxies and groups of galaxies.In The Physics of Extragalactic Radio Sources, David De Young provides a clearly written overview of what is currently known about these objects. A unique feature of the book is De Young's emphasis on the physical processes associated with extragalactic radio sources: their evolution, their environment, and their use as probes to solve other astrophysical problems. He also makes extensive use of the large amount of data now available from observations at x-ray, optical, and radio wavelengths to illustrate his main points.The Physics of Extragalactic Radio Sources will be a comprehensive introduction to the field for graduate students and a useful summary for astrophysicists.

Author Biography

Elizabeth A. Kaye specializes in communications as part of her coaching and consulting practice. She has edited Requirements for Certification since the 2000-01 edition.


Table of Contents

Preface xiii
Introduction
1(36)
Perspective
1(1)
Preliminaries
2(12)
Definitions
2(1)
Historical Note
3(1)
Names
4(1)
Techniques
5(2)
Some Physical Properties
7(7)
Morphological Types and Definitions
14(23)
Extended Sources
15(11)
Compact Objects
26(6)
Parent Objects
32(5)
Overview
37(27)
Introduction
37(1)
The Grand Questions
37(6)
What Is the Nature of the Central Engine?
37(2)
How Do Jets Form?
39(1)
What Is the Influence of the External Environment?
40(1)
What Is the Role of Nearby Objects?
41(1)
What Are the Effects of Cosmic Evolution?
42(1)
A Qualitative Picture of a Radio Source: Problems and Processes
43(21)
The Central Engine
43(6)
The Inner Jet Region
49(3)
Large Scale Jets - Basic Processes
52(10)
Radio Sources and the Environment
62(2)
Special Physical Processes
64(58)
Introduction
64(1)
Relativistic Effects
65(27)
Special Relativistic Phenomena
65(13)
General Relativistic Effects
78(14)
Radiative Processes
92(30)
Synchrotron Radiation
92(20)
Inverse Compton Radiation
112(4)
Bremsstrahlung Radiation
116(6)
Collimated Flows and Shock Waves
122(62)
Introduction
122(2)
Basic Processes in Hydrodynamics and MHD
124(34)
Conceptual Preliminaries
124(1)
Hydrodynamic Flows
125(26)
Magnetic Fields and Fluid Flows
151(7)
Mixing Layers
158(4)
Collimated Outflows and Jets
162(22)
Overview
162(2)
Mass, Momentum, and Energy Transport
164(3)
Relativistic Jets
167(3)
Some Simple Analytic Relations
170(2)
Bent Jets
172(1)
Numerical Simulations
173(11)
Microscale Processes
184(31)
Introduction
184(1)
Particle Acceleration
184(10)
Fermi Acceleration
187(2)
Acceleration at Shock Fronts
189(5)
Turbulence
194(15)
Qualitative Overview
194(3)
Some Properties of Homogeneous Incompressible Turbulence
197(6)
MHD Turbulence and Turbulent Dynamos
203(6)
The Effects of Particle Energy Losses
209(6)
Preliminaries
209(1)
Simple Evolution of Synchrotron Spectra
210(1)
Synchrotron Losses without Sources or Sinks
211(1)
Evolution of Complex Spectra
212(2)
Summary of Spectral Evolution
214(1)
Classical Double and High Luminosity Sources
215(73)
Introduction
215(5)
Overview
215(1)
An Historical Aside
216(4)
Detailed Morphology and Dynamical Indicators
220(62)
Overview of Observations
220(6)
Jets
226(35)
Hot Spots
261(8)
Lobes
269(13)
Associated Optical Properties
282(3)
Host Galaxies
282(1)
Emission Lines
283(2)
Summary of FR-II Sources
285(3)
Jets
285(1)
Hot Spots
286(1)
Lobes
287(1)
The FR-I Radio Sources
288(29)
Observational Overview
288(6)
Morphology
288(3)
Polarization Structure
291(1)
Derived Properties
292(2)
Two Exceptional FR-I Objects: 3C 120 and M87
294(10)
3C 120
295(2)
M87
297(7)
The Dynamics of FR-I Radio Sources
304(5)
Evidence for Deceleration
304(1)
Specific Models
305(3)
FR-I Dynamics: Summary
308(1)
Optical Properties
309(3)
Emission Lines
309(2)
Host Galaxies
311(1)
Comparison of FR-I and FR-II Properties
312(5)
Compact Sources
317(40)
Truly Compact Sources
318(24)
Observational Properties
319(11)
Models of GPS and CSS Sources
330(10)
The Fate of GPS and CSS Sources
340(2)
Compact Jets
342(15)
Observational Characteristics
342(7)
Blazar Models
349(6)
Compact Jets: Summary
355(2)
Unification, Models of Radio Sources
357(19)
Introduction
357(2)
Observational Clues: Evidence for Obscuration
359(2)
Specific Unification Models
361(9)
FR-II/QSO Unification
362(5)
FR-I/Blazar Unification
367(2)
Other Unifications
369(1)
Additional Aspects of Unification
370(4)
Outflow Speeds
370(1)
Possible Problems Encountered by Unification
371(3)
Perspective
374(2)
Radio Galaxies at Large Redshifts
376(60)
Introduction
376(1)
Some Cosmological Essentials
377(20)
Newtonian Cosmology
377(5)
General Relativistic Cosmologies
382(10)
Specific Cosmological Models
392(5)
High Redshift Radio Sources: Observational Characteristics
397(34)
Radio Properties
397(16)
Optical and IR Properties
413(13)
Host Galaxies
426(5)
Evolutionary Paths
431(3)
Conclusions
434(2)
Radio Sources in Galaxy Clusters
436(30)
Overview of Cluster Properties
436(10)
Definitions and Global Properties
436(2)
Dynamics
438(2)
Populations
440(3)
The Intracluster Medium
443(3)
Radio Source Properties
446(7)
Morphologies
446(2)
Statistics
448(2)
Host Galaxies
450(2)
Cluster Sources at High Redshift
452(1)
Dynamics of Head-Tail Radio Sources
453(8)
Narrow-Angle Tailed Sources
453(3)
Wide-Angle Tailed Sources
456(3)
Narrow-Angle Tails Revisited
459(1)
Head-Tail Sources in Retrospect
460(1)
Radio Galaxies and the Intracluster Medium
461(5)
Radio Halos in Clusters
461(2)
Other Implications for the Intracluster Medium
463(3)
The Central Engine
466(51)
Introduction
466(5)
A Cautionary Overview
467(4)
Black Holes - The Prime Mover
471(15)
Some General Relations
471(3)
Energy Extraction from Black Holes
474(12)
Accretion Disks - The Fueling Paradigms
486(18)
Thin Disks
487(7)
Problems with Thin Accretion Disks
494(3)
Thick Accretion Disks
497(7)
Acceleration and Collimation
504(10)
Radiative Acceleration
504(3)
Magnetohydrodynamic Processes
507(7)
Final Words
514(3)
Appendix 517(10)
References 527(24)
Index 551

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