Planetary Nebulae: International Astronomical Union Symposia, cartea 103
Editat de D.R. Floweren Limba Engleză Paperback – 30 apr 1983
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Specificații
ISBN-13: 9789027715586
ISBN-10: 9027715580
Pagini: 584
Ilustrații: 584 p. 15 illus.
Dimensiuni: 155 x 235 x 31 mm
Greutate: 0.81 kg
Ediția:Softcover reprint of the original 1st ed. 1983
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria International Astronomical Union Symposia
Locul publicării:Dordrecht, Netherlands
ISBN-10: 9027715580
Pagini: 584
Ilustrații: 584 p. 15 illus.
Dimensiuni: 155 x 235 x 31 mm
Greutate: 0.81 kg
Ediția:Softcover reprint of the original 1st ed. 1983
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria International Astronomical Union Symposia
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
Invited Papers.- Introductory Review.- Section I: Observations of Planetary Nebulae.- New and Misclassified PN.- Morphology and Kinematics of PN.- Recent Work on Bipolar Nebulae.- The Structure of the Binary Star Nebula NGC 2346.- IUE Observations of the Bipolar PN NGC 2346.- The Unprecedented Light Variations of NGC 2346.- Radio Observations of PN.- High Resolution Maps with the VLA.- Infrared Emission Lines in PN.- 10 µn Spectral Observations of Moderately Extended PN.- Molecules in PN.- Infrared Spectroscopy of the Transition Objects CRL 618 and CRL 2688.- Observations of Dust in PN.- Section II: Physical Processes in Planetary Nebulae.- Some Recent Results from UV Observations.- Recent Advances in Atomic Calculations and Experiments of Interest in the Study of PN.- Ionization Equilibrium in Models of PN.- Charge Exchange Reactions in Astrophysical Plasmas.- Recombination Processes.- Radiative Transfer Problems in PN.- Physical Processes in Nebular Shells and the Interpretation of Nebular Spectra.- On the O III/O II Problem in Medium and High Excitation PN.- PN with Massive Nuclei.- Section III: Chemical Abundances in Planetary Nebulae.- Type I PN.- Sulphur Abundances in Three Halo PN.- Elemental Abundances in PN.- Effects of Dust Formation on Chemical Abundances.- Section IV: Origin of Planetary Nebulae.- Red Giants as Precursors of PN.- Evolution of Unstable Red Giant Envelopes.- Deduction of PN Properties from Long Period Variable Precursors.- Mass Loss from Late-Type Stars: New Observational Evidence.- Effects of Stellar Mass Loss on the Formation of PN.- Fast Winds in PN.- Numerical Models of Dynamical and Spectral Evolution of PN.- Numerical Gas-Dynamic Investigation of the Whimper Model for the Formation of PN.- HBV 475 as a Candidate Proto — PN.-Comparison of PN and Symbiotic Star Emitting Regions.- Mass Loss from Central Stars of PN.- A Powerful Method for Deriving Mass-Loss Rates from PN and Other Objects: The First Order Moment W1 of Unsaturated P Cygni Line Profiles.- Influence of the Stellar Wind on the Nebular Ionization in NGC 1535 and 4361.- Section V: Central Stars of Planetary Nebulae.- Non-LTE Model Atmosphere Analysis of Central Stars.- Evolution and Mass Distribution of Central Stars of PN.- Physical Properties of the Central Stars of PN in the Magellanic Clouds.- IUE Observations of Central Stars.- Distances of the Central Stars and their Position in the HR Diagram.- The Distances of PN and the Galactic Rotation Curve.- Section VI: Planetary Nebulae an a Galactic and Extragalactic Context.- A Radio Search for Galactic Center PN.- VLA Observations of PN at the Galactic Centre.- Birthrate of PN.- PN in the Magellanic Clouds.- PN in Local Group Galaxies.- The Effects of Mass and Metallicity upon PN Formation.- PN and the Chemical Evolution of Galaxies.- PN and Seyfert Galaxies — Similarities and Differences.- Final Review.- General Discussion.- Abstracts of Contributed Papers.- Detection and Study of Secondary Structures in Some PN.- High-Spatial Resolution Observations of PN.- Kinematics of Abell 30.- A Dynamical and Chemical Study of NGC 6302.- Neutral Hydrogen Associated with the PN NGC 6302.- The Kinematical Structure of the Bipolar Nebulae M2–9 and M1–91.- High-Resolution Spectroscopy of NGC 7026.- Ionic Abundances of SIII, OIV, and NeV from Infrared Observations of Fine Structure Lines in eight PN.- Observations of the 3.3 µm Emission feature in PN.- Low-Temperature Dielectronic Recombination Coefficients for Ions of C, N and O.- Recombination Spectra of PN.- Radiative Transfer Effectsdue to Curvature and Expansion in a Dusty PN.- Profiles and Intensity Ratios of the CIV ? 1548, 1550 Emission Lines in PN.- High Dispersion IUE Observations of NGC 3918.- On the Strength of the CIV 155 nm Resonance Lines in PN.- The Formation of Resonance Lines in Gaseous Nebulae Partially Filled with Dust.- Physical Conditions in the PN Hb 12.- Physical Conditions in the Compact PN SwSt 1.- Optical and UV Nebular Spectra of NGC 40.- The Ionization Structure of NGC 6720 and NGC 7009.- Chemical Composition of the Peculiar PN YM 29.- Optically Derived Carbon Abundances in PN.- Chemical Abundance Determinations in Gaseous Nebulae.- Observations of the 30 µm feature in IRC + 10216.- OH/IR Stars: Dark PN?.- The Maser Strength of OH/IR Stars, the Evolution of Mass loss and the Formation of a PN.- Catalogue of Central Stars of PN.- Apparent Magnitudes of PN Nuclei.- UBV Observations of Variable PN.- Concerning the Temperatures of Central Stars of PN.- UV Radiation from Central Stars of PN.- Ultraviolet Spectrophotometry of Some Hotter Central Stars.- An Optical and Ultraviolet Study of Nine Low-Excitation PN.- Nebular Abundances and Central Star Parameters for eight PN in the Magellanic Clouds.- Why is IC 4642 of such a High-Excitation Class?.- Extinction — Distances to PN.- Kinematic distances of PN.- Distance Determinations from 21 cm Interstellar Absorption-Line Measurements.- OH/IR Stars Near the Galactic Centre.- Velocity Dispersion and Luminosity Function of PN in the Nuclear Bulge of M31.- Spectroscopy of the Planetary Nebula in the Fornax Galaxy with the IUE.- A New PN with Independently Determined Distance and Mass.- Spectroscopy of Extragalactic PN in the Ultraviolet.- Discovery of a Large High-Excitation PN.- Bipolar Nebulae and Type I PN.- Wind-BlanketedStellar Atmospheres.- The Temperatures of Central Stars of PN: The Energy-Balance Method.- Fabry-Pérot Radial Velocities of S274: a PN.- Three Symbiotic Stars Catalogued as PN.- Object Index.