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  • Massive Star Birth (IAU S227): A Crossroads of Astrophysics
      • GET 10% OFF

      • The discount is only available for 'Alert of Favourite Topics' newsletter recipients.
      • Publisher's listprice GBP 60.00
      • 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.

        28 665 Ft (27 300 Ft + 5% VAT)
      • Discount 10% (cc. 2 867 Ft off)
      • Discounted price 25 799 Ft (24 570 Ft + 5% VAT)

    28 665 Ft

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    Out of print

    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 23 January 2006

    • ISBN 9780521851985
    • Binding Hardback
    • No. of pages482 pages
    • Size 235x181x28 mm
    • Weight 1114 g
    • Language English
    • Illustrations 250 b/w illus.
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    Categories

    Short description:

    Proceedings of IAU S227 showing recent results and achievements in the field of massive star birth.

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    Long description:

    Massive stars, those with between 10 and 100 times the mass of the Sun, are among the rarest stars of all. They live fast and die young, but during their short lives produce the most dramatic effects on the surrounding interstellar medium in terms of dynamics, ionization, and chemical enrichment. Until a few decades ago massive star birth was literally shrouded in mystery, since these stars are born deep inside dense clouds of swirling dust and gas that obscure our view. At IAU S227, more than 200 of the world's leading astronomers presented a cornucopia of new results concerning the birth and infancy of massive stars. These proceedings show the achievements reached in this field, due to observations in the radio at mm and sub-mm wavelengths and in the infrared, and to theoretical models that simulate what happens in the cradle of a massive star.

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    Table of Contents:

    Session I: High-mass star formation near and far; Session 2: The natal precursors of OB stars; Session 3: Properties of high-mass protostars; Session 4: Massive star birth in clusters; Session 5: Ending the symposium.

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