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Dust in the Galactic Environment 2nd New edition [Mīkstie vāki]

(Rensselaer Polytechnic Institute, Troy, New York, USA)
  • Formāts: Paperback / softback, 390 pages, height x width: 235x156 mm, weight: 726 g, Contains 9 paperbacks
  • Sērija : Series in Astronomy and Astrophysics
  • Izdošanas datums: 21-Oct-2002
  • Izdevniecība: Institute of Physics Publishing
  • ISBN-10: 0750306246
  • ISBN-13: 9780750306249
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  • Mīkstie vāki
  • Cena: 101,96 €*
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  • Pievienot vēlmju sarakstam
  • Formāts: Paperback / softback, 390 pages, height x width: 235x156 mm, weight: 726 g, Contains 9 paperbacks
  • Sērija : Series in Astronomy and Astrophysics
  • Izdošanas datums: 21-Oct-2002
  • Izdevniecība: Institute of Physics Publishing
  • ISBN-10: 0750306246
  • ISBN-13: 9780750306249
Citas grāmatas par šo tēmu:
Dust is a ubiquitous feature of the cosmos, impinging directly or indirectly on most fields of modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition provides a thorough overview of the subject, covering general concepts, methods of investigation, important results and their significance, relevant literature, and some suggestions for promising avenues of future research.

Since the publication of the first edition of this popular graduate text, major advances have been made in our understanding of astrophysical dust, especially in the light of exciting new results from space- and ground-based telescopes, together with advances in laboratory astrophysics and theoretical modeling. This new, expanded edition highlights the latest results and provides a context for future research opportunities. The first chapter provides a historical perspective for current research and an overview of interstellar environments and the role of dust in astrophysical processes, followed by a discussion of the cosmic history of the chemical elements expected to be present in dust and an examination of the effect of gas-dust interactions on gas phase abundances. The next several chapters describe the observed properties of interstellar grains, such as their extinction, polarization, absorption, and emission characteristics. Then, the book explores the origin and evolution of dust, tracing its life cycle in a succession of environments from circumstellar shells to diffuse interstellar clouds, molecular clouds, protostars, and protoplanetary disks. The final chapter summarizes progress toward a unified model. Dust in other galaxies is discussed as an integral part of the text rather than as a distinct topic requiring separate chapters.

Containing extensive references and problems to aid understanding and illustrate basic principles, the book is ideally suited for graduate and advanced undergraduate courses. It will also be an invaluable reference for postgraduate students and researchers working in this important field.
Preface to the second edition xiii
Dust in the Galaxy: Our view from within
1(37)
Introduction
1(1)
Historical perspective: Discovery and assimilation
2(6)
The distribution of dust and gas
8(7)
Overview
8(2)
The galactic disc
10(2)
High galactic latitudes
12(1)
Diffuse galactic background radiation
13(2)
Interstellar environments and physical processes
15(9)
Overview
15(1)
The physical state of the interstellar medium
15(3)
Interstellar clouds
18(3)
H II regions
21(1)
The interstellar environment of the Solar System
22(2)
The significance of dust in modern astrophysics
24(4)
From Cinderella to the search for origins
24(1)
Interstellar processes and chemistry
24(2)
Stars, nebulae and galaxies
26(1)
Back to basics
27(1)
A brief history of models for interstellar dust
28(10)
Dirty ices, metals and Platt particles
29(1)
Graphite and silicates
30(3)
Unmantled refractory and core/mantle models
33(2)
Biota
35(1)
Recommended reading
35(1)
Problems
36(2)
Abundances and depletions
38(28)
The origins of the condensible elements
39(6)
The cosmic cycle: an overview
39(2)
Nucleogenesis
41(1)
Stellar nucleosynthesis
41(3)
Enrichment of the interstellar medium
44(1)
The Solar System abundances
45(5)
Significance and methodology
45(1)
Results
46(4)
Abundance trends in the Galaxy
50(4)
Temporal variation
50(1)
Spatial variation
51(2)
Solar abundances in space and time
53(1)
The observed depletions
54(7)
Methods
54(2)
Average depletions in diffuse clouds
56(3)
Dependence on environment
59(1)
Overview
60(1)
Implications for grain models
61(5)
Recommended reading
64(1)
Problems
64(2)
Extinction and scattering
66(46)
Theoretical methods
67(5)
Extinction by spherical particles
67(2)
Small-particle approximations
69(1)
Albedo, scattering function and asymmetry parameter
70(1)
Composite grains
71(1)
Observational technique
72(3)
The average extinction curve and albedo
75(9)
The average extinction curve
75(2)
Scattering characteristics
77(3)
Long-wavelength extinction and evaluation of Rv
80(2)
Neutral extinction
82(1)
Dust density and dust-to-gas ratio
83(1)
Spatial variations
84(7)
The blue-ultraviolet
84(4)
The red-infrared
88(3)
Order from chaos?
91(1)
The 2175 Å absorption feature
91(11)
Observed properties
92(5)
Implications for the identity of the carrier
97(5)
Structure in the visible
102(4)
Modelling the interstellar extinction curve
106(6)
Recommended reading
109(1)
Problems
109(3)
Polarization and grain alignment
112(42)
Extinction by anisotropic particles
113(2)
Polarimetry and the structure of the galactic magnetic field
115(10)
Basics
115(2)
Macroscopic structure
117(3)
Polarization efficiency
120(2)
Small-scale structure
122(1)
Dense clouds and the skin-depth effect
123(2)
The spectral dependence of polarization
125(13)
The Serkowski law
125(2)
Power-law behaviour in the infrared
127(1)
Polarization and extinction
128(4)
Regional variations
132(5)
Circular polarization
137(1)
Polarization and grain models
138(3)
Alignment mechanisms
141(13)
Grain spin and rotational dissipation
142(3)
Paramagnetic relaxation: the DG mechanism
145(2)
Superparamagnetic alignment
147(1)
Suprathermal spin
148(1)
Radiative torques
149(1)
Mechanical alignment
150(1)
Alignment in dense clouds
151(1)
Recommended reading
152(1)
Problems
152(2)
Infrared absorption features
154(41)
Basics of infrared spectroscopy
155(7)
Vibrational modes in solids
155(4)
Intrinsic strengths
159(1)
Observational approach
160(2)
The diffuse ISM
162(12)
The spectra
162(3)
Silicates
165(4)
Silicon carbide
169(1)
Hydrocarbons and organic residues
170(4)
The dense ISM
174(21)
An inventory of ices
174(2)
The threshold effect
176(2)
H2O-ice: the 3 μm profile
178(3)
Solid CO: polar and apolar mantles
181(1)
Other carbon-bearing ices
182(3)
Nitrogen and sulphur-bearing ices
185(2)
Refractory dust
187(3)
Spectropolarimetry and alignment of core-mantle grains
190(3)
Recommended reading
193(1)
Problems
193(2)
Continuum and line emission
195(31)
Theoretical considerations
196(8)
Equilibrium dust temperatures
196(2)
FIR continuum emission from an interstellar cloud
198(2)
Effect of grain shape
200(2)
Effect of grain size
202(2)
Galactic continuum emission
204(8)
Morphology
204(1)
Spectral energy distribution
204(3)
Dust and gas
207(3)
The `cold dust problem'
210(1)
Polarization and grain alignment
210(2)
Spectral emission features
212(10)
Silicates
212(2)
Polycyclic aromatic hydrocarbons
214(8)
Extended red emission
222(4)
Recommended reading
224(1)
Problems
225(1)
Dust in stellar ejecta
226(37)
The formation of dust in stellar outflows
227(8)
Theoretical considerations
227(2)
The circumstellar environment
229(1)
O-rich stars
230(2)
Carbon stars
232(2)
Late stages of stellar evolution
234(1)
Observational constraints on stardust
235(17)
Infrared continuum emission
235(3)
Infrared spectral features
238(7)
Circumstellar extinction
245(2)
Stardust in meteorites
247(5)
Evolved stars as sources of interstellar grains
252(11)
Mass-loss
252(3)
Grain-size distribution
255(1)
Dust-to-gas ratio
256(1)
Composition
257(1)
Injection rate
257(4)
Recommended reading
261(1)
Problems
261(2)
Evolution in the interstellar medium
263(32)
Grain surface reactions and the origin of molecular hydrogen
264(4)
Gas-phase chemistry
268(3)
Mechanisms for growth
271(4)
Coagulation
272(1)
Mantle growth
273(2)
Ice mantles: deposition and evolution
275(12)
Surface chemistry and hierarchical growth
275(2)
Depletion timescales and limits to growth
277(2)
Thermal and radiative processing
279(8)
Refractory dust
287(8)
Destruction
287(3)
Size distribution
290(1)
Metamorphosis
291(1)
Dust in galactic nuclei
292(1)
Recommended reading
293(1)
Problems
293(2)
Dust in the envelopes of young stars
295(37)
The early phases of stellar evolution
296(10)
Overview
296(2)
Infrared emission from dusty envelopes
298(4)
Polarization and scattering
302(2)
Ice sublimation in hot cores
304(2)
Protoplanetary discs
306(6)
T Tauri discs
307(1)
Vega discs
308(2)
The solar nebula
310(2)
Clues from the early Solar System
312(10)
Comets
313(5)
Interplanetary dust
318(2)
Meteorites
320(2)
Ingredients for life
322(10)
Motivation
322(1)
The deuterium diagnostic
323(2)
Amino acids and chirality
325(3)
Did life start with RNA?
328(1)
Delivery to Earth
329(2)
Recommended reading
331(1)
Problems
331(1)
Toward a unified model for interstellar dust
332(8)
Areas of consensus
333(4)
A generic grain model
333(2)
Silicates
335(1)
Carbon
335(1)
Ices
336(1)
Alignment
336(1)
Open questions
337(3)
A Glossary 340(8)
Units and constants
340(1)
Physical, chemical and astrophysical terms
341(5)
Acronyms
346(2)
References 348(30)
Index 378