ISBN: 9789401134026
Light scattering and absorption by small homogeneous particles can be worked-out exactly for spheres and infinite cylinders. Homogeneous particles of irregular shapes, when averaged with … Meer...
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ISBN: 9789401134026
Light scattering and absorption by small homogeneous particles can be worked-out exactly for spheres and infinite cylinders. Homogeneous particles of irregular shapes, when averaged with … Meer...
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ISBN: 9789401134026
Light scattering and absorption by small homogeneous particles can be worked-out exactly for spheres and infinite cylinders. Homogeneous particles of irregular shapes, when averaged with … Meer...
ISBN: 9789401134026
Light scattering and absorption by small homogeneous particles can be worked-out exactly for spheres and infinite cylinders. Homogeneous particles of irregular shapes, when averaged with … Meer...
2012
ISBN: 9789401134026
eBook Download (PDF), eBooks, [PU: Springer Netherlands]
2012, ISBN: 9789401134026
eBook Download (PDF), eBooks, [PU: Springer]
ISBN: 9789401134026
eBooks > Belletristik > Erzählungen
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Gedetalleerde informatie over het boek. - Theory of Cosmic Grains
EAN (ISBN-13): 9789401134026
Verschijningsjaar: 2012
Uitgever: Springer Netherlands
Boek bevindt zich in het datenbestand sinds 2017-05-22T23:21:10+02:00 (Amsterdam)
Detailpagina laatst gewijzigd op 2021-10-04T19:45:15+02:00 (Amsterdam)
ISBN/EAN: 9789401134026
ISBN - alternatieve schrijfwijzen:
978-94-011-3402-6
alternatieve schrijfwijzen en verwante zoekwoorden:
Auteur van het boek: wickram, wickrama, wickramasinghe
Gegevens van de uitgever
Auteur: N.C. Wickramasinghe; B. Hoyle
Titel: Astrophysics and Space Science Library; The Theory of Cosmic Grains
Uitgeverij: Springer; Springer Netherland
307 Bladzijden
Verschijningsjaar: 2012-12-06
Dordrecht; NL
Taal: Engels
149,79 € (DE)
154,00 € (AT)
177,00 CHF (CH)
Available
IX, 307 p.
EA; E107; eBook; Nonbooks, PBS / Physik, Astronomie/Astronomie; Astronomische Beobachtung: Observatorien, Ausrüstungen und Methoden; Verstehen; Galaxy; galaxies; stellar; C; Astronomy, Observations and Techniques; Physics and Astronomy; BB
1. Introduction.- 1.1. Early Ideas.- 1.2. Trumpler’s Method of Estimating Interstellar Extinction.- 1.3. The First Colour Measurements.- 1.4. The Oort Limit.- 1.5. Data Relating to Interstellar Clouds.- 1.6. Correlation Between Gas and Dust Clouds.- 1.7. Composition of Grains.- 2. Electromagnetic Properties of Small Particles.- 2.1. Homogeneous Spherical Particles.- 2.2. Composite Spheres.- 2.3. Infinite Cylinders.- 2.4. Rayleigh Scattering by Ellipsiods.- 2.5. Heterogeneous or Porous Grains.- 2.6. Absorption Cross—sections, Bulk Absorption Coefficient and Emissivity.- 2.7. Two Special Cases.- 3. Interstellar Extinction and Polarisation.- 3.1. Equation of Transfer.- 3.2. Observations of Interstellar Extinction, Definition of Colour Indices and Colour Excesses.- 3.3. Observations of Interstellar Polarisation.- 3.4. Diffuse Interstellar Bands.- 4. Reflection Nebulae and the Diffuse Galactic Light.- 4.1. Introductory Remarks.- 4.2. Apparent Size of Reflection Nebulae.- 4.3. Observations of NGC 7023.- 4.4. Observations of Reflection Nebula Around Merope.- 4.5. Multiple Scattering Models of Reflection Nebulae.- 4.6. Diffuse Galactic Light.- 5 Interactions between Dust, Gas and Radiation.- 5.1.Introductory Remarks.- 5.2. Grain Temperatures for Sandard Grains.- 5.3.Temperature Spikes in Very Small Grains.- 5.4.Electrostatic Gharge on Grains.- 5.5.Rotation of Grains.- 5.6.Radio Waves from Grains.- 5.7.Molecule Formation.- 5.8. Growth and Destruction of Grains.- 5.9. Effects of Radiation Pressure.- 5.10. Gyration About the Magnetic Field.- 5.11. Alignment of Grains.- 5.12. Depletion of Elements from the Gas Phase.- 6. Inorganic Theories of Grain Formation.- 6.1. Interstellar Condensation.- 6.2. Condensation of Graphite Grains.- 6.3. Condensation of Grains in CoolOxygen—rich Giant Stars.- 6.4. Core—mantle Grains.- 7. The Organic Grain Model.- 7.1. Introductory Remarks.- 7.2. Polymerisation of Formaldehyde.- 7.3. From Formaldehyde to Polysacharides.- 7.4. Polysacharide Formation in Stellar Mass Flows.- 7.5. HAC, PAH and QCC Models.- 7.6. Fischer Tropsch Reactions in the Gas Phase.- 7.7. The Biological Grain Model.- 8. Models of the Extinction and Polarisation of Starlight.- 8.1. Introduction.- 8.2. The Visual Extinction Curve.- 8.3. The Ultraviolet Extinction Curve: Extinction Curves for Graphite Grains.- 8.4. Polarisation Constraints.- 8.5. An Organic/Biologic Grain Model.- 8.6. Analysis of a Biological Grain Model.- 8.7. Refinements to Biological Extinction Model.- 9. Spectroscopic Identifications.- 9.1. Introduction.- 9.2. The 8 – 13µm Features in Astronomy.- 9.3. The 8 – 40µm Flux from the Trapezium Nebula.- 9.4. The 3.4µm Band: Proof that Grains are Mainly Organic.- 9.5. Modelling the 2.9 – 4µm IR Data for GC-IRS7.- 9.6. How Much Water — Ice?.- 9.7. Sources with Spectra in the 2 – 14µm Waveband.- 9.8. Evidence for PAH.- 9.9. Aromatic Molecules and the Diffuse Optical Bands.- 10. Dust in External Galaxies.- 10.1. Introduction.- 10.2. The Magellanic Clouds: LMC and SMC.- 10.3. M82 and Other Galaxies.- 10.4. Particles of High Infrared Emissivity.- 10.5. The Ejection of Iron Whiskers from Galaxies.- 10.6. The Microwave Background.Andere boeken die eventueel grote overeenkomsten met dit boek kunnen hebben:
Laatste soortgelijke boek:
9789401134033 Theory of Cosmic Grains (N C Wickramasinghe; B Hoyle)
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