Polycyclic Aromatic Hydrocarbons and Astrophysics - nieuw boek

EAN (ISBN-13): 9789401086196
ISBN (ISBN-10): 9401086192
Gebonden uitgave
pocket book
Verschijningsjaar: 2011
Uitgever: Springer

Boek bevindt zich in het datenbestand sinds 2014-10-10T19:46:46+02:00 (Amsterdam)
Detailpagina laatst gewijzigd op 2023-11-15T20:06:51+01:00 (Amsterdam)
ISBN/EAN: 9401086192

ISBN - alternatieve schrijfwijzen:
94-010-8619-2, 978-94-010-8619-6
alternatieve schrijfwijzen en verwante zoekwoorden:
Auteur van het boek: léger, leger, boccara
Titel van het boek: hydrocarbon, hydrocarbons

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Gegevens van de uitgever

Auteur: A. Léger; L. D'Hendecourt; N. Boccara
Titel: Nato Science Series C:; Polycyclic Aromatic Hydrocarbons and Astrophysics
Uitgeverij: Springer; Springer Netherland
402 Bladzijden
Verschijningsjaar: 2011-09-26
Dordrecht; NL
Gedrukt / Gemaakt in
Taal: Engels
213,99 € (DE)
219,99 € (AT)
236,00 CHF (CH)
POD
XV, 402 p.

BC; Hardcover, Softcover / Physik, Astronomie/Astronomie; Astronomische Beobachtung: Observatorien, Ausrüstungen und Methoden; Verstehen; Galaxy; astrophysics; galaxies; interstellar matter; planet; spectroscopy; stellar; universe; Astronomy, Observations and Techniques; BB; EA

Section 1: Introduction.- Objectives of the Workshop.- Photons, Molecules and Solids in Interstellar and Circumstellar Regions: an Introduction for Non-Astronomers.- Section 2: Physics and Chemistry of Graphite, Carbonaceous Grains and Clusters.- On the Electronic Structure of Graphite.- Various Kinds of Solid Carbon: Structure and Optical Properties.- Gas/Carbonaceous Surface Interactions.- VUV to FIR Laboratory Observations on Submicron Amorphous Carbon Particles.- Spectroscopy of Matrix-Isolated Carbon Molecules in the UV, VIS, and IR Spectral Range.- Remarkable Periodicities in the Mass Spectra of Carbon Aggregates.- Reactions of Thermal Hydrogen Atoms and Energetic Hydrogen and Oxygen Ions with Pyrolytic Graphite.- Section 3: Physics and Chemistry of Polycyclic Aromatic Hydrocarbons (Pah’s).- Photophysics, Electronic Spectroscopy and Relaxation of Molecular Ions and Radicals with Special Reference to Polycyclic Aromatic Hydrocarbons.- Fluorescence Lineshapes of Polyatomic Molecules — Spectroscopy without Eigenstates.- Structure and Chemistry of PAH’s.- Synthesis and Spectroscopy of Tribenzo(a, g, m)Coronene, a New, Exceptionally Stable, Fully Benzenoid PAH.- Hot Carbon Atoms as a Potential Source for Polycyclic Aromatic Hydrocarbons.- Section 4: Carbonaceous Materials and Astrophysics.- Carbon Components of Interstellar Dust.- Molecular Origin of the 216 nm Interstellar Hump.- Chains and Grains in Interstellar Space.- Mid Infrared Excess and Ultraviolet Extinction.- High Spectral Resolution Observation of the 3.3 ?m Emission Band and Comparison with Laboratory-Synthesized Quenched Carbonaceous Composite (QCC).- DISCUSSION I: Carbon in the Interstellar Medium.- Section 5: Polycyclic Aromatic Hydrocarbons and Astrophysics.- Identification of PAH’s inAstronomical IR Spectra — Implications.- The IR Emission Features: Emission from PAH Molecules and Amorphous Carbon Particles.- The Hydrogen Coverage of Interstellar PAH’s.- New Observations of Infrared Astronomical Bands: IRAS-LRS and 3 ?rn Ground-Based Spectra.- Distribution of PAH in the Galaxy Derived from the IRAS Data.- Infrared Features in Extragalactic Objects.- Very Small Grains in Spiral Galaxies.- IRAS Observations of a “Typical” Dark Cloud.- Coal Tar as a Laboratory Analog of an Interstellar PAH Mixture.- Hydrogenated Amorphous Carbon (a:C-H) in the Planetary Nebula NGC 7027.- Visual and Infrared Fluorescence from L1780.- DISCUSSION II: Interpretation of IR Observations.- Section 6: Diffuse Interstellar Bands.- Possible Carriers of the Diffuse Interstellar Bands.- DISCUSSION III: The Diffuse Interstellar Bands. Are they Carried by PAH’s?.- Section 7: Physics and Chemistry of Pah’s in the Interstellar Medium.- Physics and Chemistry of Interstellar Polycyclic Aromatic Molecules.- Formation, Destruction and Excitation of Carbon Grains and PAH Molecules.- Polyaromatic Hydrocarbons and the Condensation of Carbon in Stellar Winds.