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9780691004020

Galactic Astronomy

by ;
  • ISBN13:

    9780691004020

  • ISBN10:

    0691004021

  • Format: Hardcover
  • Copyright: 1998-09-01
  • Publisher: Princeton Univ Pr
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Supplemental Materials

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Summary

This is the definitive treatment of the phenomenology of galaxies--a clear and comprehensive volume that takes full account of the extraordinary recent advances in the field. The book supersedes the classic text Galactic Astronomy that James Binney wrote with Dimitri Mihalas, and complements Galactic Dynamics by Binney and Scott Tremaine. It will be invaluable to researchers and is accessible to any student who has a background in undergraduate physics. The book draws on observations both of our own galaxy, the Milky Way, and of external galaxies. The two sources are complementary, since the former tends to be highly detailed but difficult to interpret, while the latter is typically poorer in quality but conceptually simpler to understand. Binney and Merrifield introduce all astronomical concepts necessary to understand the properties of galaxies, including coordinate systems, magnitudes and colors, the phenomenology of stars, the theory of stellar and chemical evolution, and the measurement of astronomical distances. The book's core covers the phenomenology of external galaxies, star clusters in the Milky Way, the interstellar media of external galaxies, gas in the Milky Way, the structure and kinematics of the stellar components of the Milky Way, and the kinematics of external galaxies. Throughout, the book emphasizes the observational basis for current understanding of galactic astronomy, with references to the original literature. Offering both new information and a comprehensive view of its subject, it will be an indispensable source for professionals, as well as for graduate students and advanced undergraduates.

Table of Contents

Preface xii
1 Galaxies: an overview
1(25)
1.1 Introduction
1(1)
1.2 A brief history of galactic astronomy
2(24)
Photometric models of the Milky Way
5(5)
The nature of the spiral nebulae
10(5)
Kinematic models of the Milky Way
15(5)
Stellar populations
20(1)
More recent developments
21(5)
2 Astronomical Measurements
26(50)
2.1 Positions, motions and coordinate systems
27(11)
The equatorial system
27(3)
Galactic coordinates
30(1)
Parallax
31(3)
Proper motions
34(1)
Precession and nutation
35(2)
Astrometric systems
37(1)
2.2 Distances determined from velocities
38(8)
Radial velocities
39(1)
Distances from the moving-cluster method
40(2)
Secular parallaxes
42(3)
Statistical parallaxes
45(1)
2.3 Magnitudes and colors
46(16)
Apparent magnitudes
47(5)
Colors
52(4)
Absolute magnitudes
56(2)
Absolute energy distributions and bolometric magnitudes
58(2)
Mass-to-light ratios
60(1)
Surface brightness and isophotal radii
61(1)
2.4 Gravitational lensing
62(5)
2.5 Archival data and catalogs
67(7)
On-line resources
71(3)
Problems
74(2)
3 The Properties of Stars
76(69)
3.1 The masses of stars
76(6)
The Mass of the Sun
77(1)
Masses of binary stars
78(1)
Visual binaries
78(1)
Spectroscopic binaries
79(3)
3.2 The radii of stars
82(5)
Phase interferometry
82(1)
Intensity interferometry
83(1)
Speckle interferometry
83(1)
Lunar occultations
84(1)
Eclipsing binaries
84(2)
Astrophysical estimates
86(1)
3.3 Classification of stars
87(7)
Novae
87(1)
Pulsars
87(1)
Classification of stellar spectra
88(2)
The MK System
90(4)
3.4 Physical interpretation of stellar spectra
94(8)
3.5 Color-magnitude diagrams
102(7)
Observed CM-diagrams
103(1)
Luminosity and color as functions of spectral class
104(5)
The physical properties of stars on the MS and RGB
109(1)
3.6 The stellar luminosity function
109(22)
Malmquist bias
111(4)
Lutz-Kelkar Bias
115(4)
The general luminosity function
119(1)
Cluster luminosity functions
119(1)
Photometrically complete surveys
119(1)
Proper-motion selected surveys
120(7)
The luminosity function of a given MK spectral class
127(3)
Catalogs of the nearby stars
130(1)
3.7 Interstellar dust
131(12)
Extinction and reddening
133(5)
Reddening-free indices
138(2)
Polarization of starlight by dust
140(1)
Extinction of sight-lines out of the Galaxy
140(3)
Problems
143(2)
4 Morphology of Galaxies
145(113)
4.1 Morphological classification of galaxies
146(26)
The Hubble sequence
149(8)
Effects of environment
157(5)
The galaxy luminosity function
162(1)
The field galaxy luminosity function
162(3)
The cluster galaxy luminosity function
165(2)
The luminosity function divided by morphological type
167(2)
The Local Group
169(3)
4.2 Surface Photometry of Galaxies
172(13)
The night sky
173(3)
Effect of seeing
176(3)
Deprojecting galaxy images
179(6)
4.3 Photometry of Elliptical Galaxies
185(25)
Radial surface-brightness profiles of elliptical galaxies
185(1)
cD galaxies
186(4)
Dwarf elliptical galaxies
190(1)
Centers of elliptical galaxies
191(2)
Color and line-strength gradients in elliptical galaxies
193(1)
Shapes of elliptical galaxies
194(1)
Ellipticity
194(5)
Deviations from ellipses
199(2)
Fine structure
201(3)
Correlations among global parameters of elliptical galaxies
204(5)
The D(n) - theta (0) correlation
209(1)
Dwarf elliptical galaxies
209(1)
4.4 Photometry of Disk Galaxies
210(25)
Photometric effects of dust
211(1)
Overall shapes of disk galaxies
212(2)
Bulge-disk decomposition
214(8)
Shapes of bulges
222(1)
Color and metallicity gradients in disk galaxies
223(1)
Spiral structure in disk galaxies
224(4)
Barried galaxies
228(3)
Vertical structure of bars
231(2)
Rings in SB galaxies
233(1)
Dust lanes in SB galaxies
234(1)
Lop-sidedness in SB galaxies
234(1)
4.5 Globular cluster systems
235(6)
Globular cluster luminosity function
236(1)
Specific frequency of globular clusters
237(1)
Radial density profiles and shapes
238(1)
Color distributions
239(2)
4.6 Abnormal galaxies
241(14)
Starbursting systems
241(3)
Systems with active galactic nuclei
244(6)
Host galaxies of AGN
250(1)
The unified model of AGN
251(4)
Problems
255(3)
5 Evolution of Stars and Stellar Populations
258(69)
5.1 Stellar evolution and the CM diagram
259(37)
Placing models in the CM diagram
262(1)
Features in the CM diagram
263(4)
Characteristic initial masses
267(7)
Bounding curves in the CM diagram
274(2)
Dependence of CM diagrams upon metallicity
276(3)
The cosmic helium abundance
279(1)
Simple numerical relations
279(2)
Star formation
281(2)
The initial mass function
283(4)
Pulsating stars
287(2)
Classical Cepheid variables
289(3)
Mira variables
292(1)
W Virginis stars
293(1)
RR Lyrae stars
293(3)
5.2 Synthesis of the chemical elements
296(10)
Basic nuclear physics
296(5)
Metal production at M(i) is less than M(up)
301(1)
Supernovate
302(1)
Metal production by core-collapse supernovae
303(2)
Metal production by type Ia supernovae
305(1)
5.3 Models of chemical enrichment
306(8)
The closed-box model
306(2)
The leaky-box model
308(5)
The accreting-box model
313(1)
5.4 Evolution of stellar populations
314(10)
Analytical results
315(2)
Numerical models of populations evolution
317(7)
Problems
324(3)
6 Star clusters
327(67)
6.1 Globular clusters
327(50)
Globular cluster steller photometry
332(2)
Color-magnitude diagrams
334(1)
The main sequence and subgiant branch
335(2)
The horizontal branch
337(2)
Comparison with Theoretical CM diagrams
339(5)
Globular cluster ages
344(1)
Turnoff point ages
344(1)
Isochrone fitting
345(1)
The delta V method
346(1)
The Delta (B - V) method
347(1)
Comparison with the age of the Universe
348(1)
Variations in age
349(1)
Metallicities of globular clusters
350(1)
Omega cen
351(1)
The third parameter problem
352(1)
Variations in helium abundance
353(1)
Variations in other element abundances
353(1)
Other candidates
354(1)
Luminosity functions
354(5)
Binary stars
359(2)
Stellar remnants
361(1)
White dwarfs
361(1)
Neutron stars
362(1)
Radial profiles
363(2)
Large-scale properties
365(2)
Luminosity segregation
367(2)
Central cusps
369(2)
Kinematics
371(3)
Velocities of individual stars
371(3)
Integrated-light kinematics
374(1)
Proper motions
375(2)
6.2 Open clusters
377(15)
Color-magnitude diagrams
381(3)
The ages and demise of open clusters
384(2)
Structure and kinematics
386(3)
Luminosity function
389(3)
Problems
392(2)
7 The Cosmic Distance Scale
394(57)
7.1 An introduction to cosmology
396(3)
7.2 Absolute distance estimators
399(15)
The Baade-Wesselink method
399(3)
Application to supernovae
402(1)
The Sunyaev-Zel'dovich effect
403(2)
Distances from time delays
405(1)
The ring around Supernova 1987A
406(1)
Gravitational lens time delays
407(3)
Water-master proper-motions by VLBI
410(4)
7.3 Relative distance estimators
414(15)
Luminosities of variable stars
415(1)
Luminosity functions
415(1)
Globular clusters
416(1)
Planetary nebulae
417(2)
Novae and supernovae
419(1)
Novae
419(1)
Type Ia supernovae
420(2)
Distances from galaxy kinematics
422(1)
Spiral galaxies
422(3)
Elliptical galaxies
425(1)
Surface brightness fluctuations
426(3)
7.4 Results
429(20)
Distance within the Local Group
432(1)
Distance to the Galactic center
432(2)
Distance to the Large Magellanic Cloud
434(1)
Distance to M31
435(2)
Distance beyond the Local Group
437(1)
Distance to the Virgo Cluster
437(2)
Peculiar velocity field
439(2)
The asymptotic Hubble constant
441(3)
The deceleration parameter and cosmic density
444(1)
Standard candles and rulers
444(3)
Peculiar velocity field
447(2)
Problems
449(2)
8 The Interstellar Media of Galaxies
451(84)
8.1 How interstellar matter is detected
452(36)
Absorption of starlight
452(7)
Extreme UV and X-ray observations
459(4)
Optical emission lines
463(1)
Hydrogen lines
463(1)
Metal lines
464(4)
Radio observations
468(3)
The 21-cm line of atomic hydrogen
471(3)
Rotation transitions of heteronuclear molecules
474(4)
Synchrotron radiation
478(2)
Radio-frequency bremsstrahlung and recombination lines
480(1)
Dispersion and Rotation Measures
481(1)
Gamma-ray emission
482(1)
Radiation by dust
483(5)
8.2 The ISM in Disk Galaxies
488(37)
Global measures
493(1)
HI and H(2) in disk galaxies
493(3)
Radio-continuum and IR luminosities
496(2)
Radial density profiles
498(2)
Azimuthal distributions
500(1)
Bars and oval distortions
500(1)
Spiral structure
500(2)
Lop-sidedness
502(3)
Velocity fields of disks
505(2)
Circular-speed curves
507(3)
Kinematic warps
510(2)
Oval distortions
512(1)
So galaxies
513(3)
Metallicities of disk galaxies
516(4)
Magnetic fields
520(2)
Star formation in disk galaxies
522(3)
8.3 The ISM in elliptical galaxies
525(5)
X-ray emitting plasma
525(2)
Cool gas in ellipticals
527(5)
8.4 Intergalactic gas
530(3)
The Magellanic Stream
530(3)
Problems
533(2)
9 The Milky Way's ISM
535(71)
9.1 The kinematics of differential rotation
536(13)
The naive (l,v) plot
536(4)
Radii and distances from the (l,v) plot
540(1)
Non-circular motion and the (l,v) plot
541(1)
Axisymmetric expansion
541(1)
Oval distortions
542(2)
Spiral structure
544(2)
Random motions
546(3)
9.2 The large-scale distribution of HI and CO
549(21)
The 21-cm line in emission
549(4)
Measuring the spin temperature
553(1)
CO lines in emission
554(1)
The Milky Way's circular-speed curve
555(4)
Radial distributions of HI and CO
559(2)
Evidence for spiral structure
561(1)
Vertical distributions of HI and CO
562(1)
The middle disk
563(2)
The outer disk
565(5)
9.3 Other tracers of the ISM
570(10)
Diffuse infrared emission
570(4)
Pulsars and the Galactic magnetic field
574(2)
Diffuse H Alpha radiation
576(1)
Diffuse synchrotron and Gamma-radiations
577(2)
Diffuse X-rays
579(1)
9.4 The central disk
580(14)
21-cm observations
580(6)
Observations in lines of CO and CS
586(2)
A dynamical model of the central disk
588(6)
9.5 The nucleus
594(3)
9.6 Small-scale structure of the ISM
597(6)
Molecular gas in the Galaxy
598(3)
X from virial masses
601(1)
X from Gamma-rays
601(1)
X from A(V)
602(1)
Problems
603(3)
10 Components of the Milky Way
606(87)
10.1 Gross Structure from Surface Photometry
609(7)
The Galaxy at optical wavelengths
614(2)
10.2 The bulge
616(8)
Integrated surface photometry
616(3)
Evidence for a bar from individual stars
619(2)
Age and metallicity of the bulge
621(1)
Bulge kinematics
622(2)
10.3 Kinematics of stars near the Sun
624(19)
The solar motion
624(5)
Random velocities of stars
629(1)
Vertex deviation
630(2)
The Schwarzchild distribution
632(2)
Star streams
634(2)
Causes of vertex deviation
636(1)
The Oort constants
637(4)
Estimating the Oort constants
641(2)
10.4 The structure of the stellar disk
643(23)
Ages and metallicities of nearby stars
643(1)
Correlations between abundances
643(1)
Correlations between age and abundance
644(7)
The old disk clusters
651(1)
Stars counts and the thick disk
651(3)
The thick disk
654(2)
The local mass density of the disk
656(8)
Distribution of the youngest stars
664(2)
10.5 The halo
666(12)
The globular cluster system
666(4)
Field halo stars
670(3)
Kinematically selected samples
673(5)
10.6 Galaxy models
678(6)
The local circular speed
679(1)
Mass models
680(2)
Starcount models
682(1)
Kinematic models
683(1)
Dynamical models
683(1)
10.7 Formation and evolution of the Milky Way
684(6)
Formation scenarios
684(4)
Models of the chemical evolution of the Milky Way
688(1)
Chemical evolution of the halo
688(1)
Pre-enrichment
688(2)
Problems
690(3)
11 Stellar Kinematics in External Galaxies
693(39)
11.1 Measuring the kinematics of external galaxies
694(13)
Mean velocities and velocity dispersion
697(3)
Analysis of line profiles
700(5)
Position-velocity diagrams and data cubes
705(2)
11.2 The stellar kinematics of elliptical galaxies
707(15)
Large-scale properties
707(1)
Major-axis kinematics
707(5)
Detection of dark halos
712(1)
Kinematic mapping
713(3)
Core properties
716(1)
Decoupled cores
716(1)
Detection of central black holes
717(5)
11.3 The stellar kinematics of disk galaxies
722(8)
Bulge kinematics
723(1)
Disk kinematics
724(1)
Rotational motion
725(2)
Random motions
727(3)
Problems
730(2)
Appendices 732(13)
A Gravitational deflection of light 732(4)
B Important astronomical catalogs 736(7)
C Richardson-Lucy deconvolution 743(1)
D Useful numbers 744(1)
References 745(32)
Index 777

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