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Herausgeber: 
  • Diego F. Torres
  • Modelling Pulsar Wind Nebulae 
     

    (Buch)
    Dieser Artikel gilt, aufgrund seiner Grösse, beim Versand als 5 Artikel!


    Übersicht

    Auf mobile öffnen
     
    Lieferstatus:   Auf Bestellung (Lieferzeit unbekannt)
    Veröffentlichung:  November 2017  
    Genre:  Naturwissensch., Medizin, Technik 
     
    Astronomy, Observations and Techniques / Astronomy, space & time / Astronomy—Observations / Astrophysics / Astrophysics and Astroparticles / B / Mathematical physics / Mathematische Physik
    ISBN:  9783319630304 
    EAN-Code: 
    9783319630304 
    Verlag:  Springer EN 
    Einband:  Gebunden  
    Sprache:  English  
    Serie:  #446 - Astrophysics and Space Science Library  
    Dimensionen:  H 235 mm / B 155 mm / D 27 mm 
    Gewicht:  6151 gr 
    Seiten:  313 
    Illustration:  XI, 313 p. 121 illus., 105 illus. in color., farbige Illustrationen, schwarz-weiss Illustrationen 
    Zus. Info:  EUDR exemption - product or manufacturing materials placed on the market prior to 31.12.2025. 
    Bewertung: Titel bewerten / Meinung schreiben
    Inhalt:
    In view of the current and forthcoming observational data on pulsar wind nebulae, this book offers an assessment of the theoretical state of the art of modelling them. The expert authors also review the observational status of the field and provide an outlook for future developments.

    During the last few years, significant progress on the study of pulsar wind nebulae (PWNe) has been attained both from a theoretical and an observational perspective, perhaps focusing on the closest, more energetic, and best studied nebula: the Crab, which appears in the cover. Now, the number of TeV detected PWNe is similar to the number of characterized nebulae observed at other frequencies over decades of observations. And in just a few years, the Cherenkov Telescope Array will increase this number to several hundreds, actually providing an essentially complete account of TeV emitting PWNe in the Galaxy. At the other end of the multi-frequency spectrum, the SKA and its pathfinder instruments, will reveal thousands of new pulsars, and map in exquisite detail the radiation surrounding them for several hundreds of nebulae.

    By carefully reviewing the state of the art in pulsar nebula research this book prepares scientists and PhD students for future work and progress in the field.

      
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