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  • Planetary Nebulae in our Galaxy and Beyond (IAU S234): Proceedings of the 234th Symposium of the International Astronomical Union Held in Waikoloa Beach, Hawaii, USA April 3-7, 2006

    Planetary Nebulae in our Galaxy and Beyond (IAU S234) by Méndez, Roberto H.; Barlow, Michael J.;

    Proceedings of the 234th Symposium of the International Astronomical Union Held in Waikoloa Beach, Hawaii, USA April 3-7, 2006

    Series: Proceedings of the International Astronomical Union Symposia and Colloquia;

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      • Publisher's listprice GBP 81.00
      • The price is estimated because at the time of ordering we do not know what conversion rates will apply to HUF / product currency when the book arrives. In case HUF is weaker, the price increases slightly, in case HUF is stronger, the price goes lower slightly.

        38 697 Ft (36 855 Ft + 5% VAT)
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    Estimated delivery time: In stock at the publisher, but not at Prospero's office. Delivery time approx. 3-5 weeks.
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    Why don't you give exact delivery time?

    Delivery time is estimated on our previous experiences. We give estimations only, because we order from outside Hungary, and the delivery time mainly depends on how quickly the publisher supplies the book. Faster or slower deliveries both happen, but we do our best to supply as quickly as possible.

    Product details:

    • Publisher Cambridge University Press
    • Date of Publication 5 February 2007

    • ISBN 9780521863438
    • Binding Hardback
    • No. of pages590 pages
    • Size 253x180x32 mm
    • Weight 1327 g
    • Language English
    • Illustrations 250 b/w illus. 110 tables
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    Short description:

    IAU S234 summarises current research on planetary nebulae, in reviews by leading experts in the field.

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    Long description:

    Planetary nebulae represent the brief transition between Asymptotic Giant Branch stars and White Dwarfs. As multi-wavelength laboratories they have played a key role in developing our understanding of atomic, molecular, dust and plasma processes in astrophysical environments. The means by which their wonderfully diverse morphologies are obtained is currently the subject of intense research, including hydrodynamical shaping mechanisms and the role of binarity, stellar magnetic fields and rotation. Their contribution to the chemical enrichment of galaxies is another very active research area, as is the ever growing use of their narrow high luminosity emission lines to probe the dynamics and mass distributions of galaxies and the intergalactic media of clusters of galaxies. IAU S234 summarises the current status of research on the properties and processes of planetary nebulae, as reported in reviews and papers by leading experts working in the field.

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    Table of Contents:

    Preface; Part I. Invited Reviews and Contributed Presentations: A. Surveys for planetary nebulae; B. Distances, AGB stars and post-AGB objects; C. Post-AGB objects, nucleosynthesis and central stars; D. Central star properties; E. Multi-wavelength properties of the nebulae; F. Physical properties, nebular abundances; G. Abundances, formation of nebular structures; H. Nebular structures, Magellanic Cloud planetary nebulae; I. Extragalactic planetary nebulae; Part II. Poster Presentations; Indices.

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