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Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories

Modern astrophysics is a mature science that has evolved from its early phase of discovery and classification to a physics-oriented discipline focused in finding answers to fundamental problems ranging from cosmology to the origin and diversity of life-sustainable systems in the Universe. For this v...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor Corporativo: SpringerLink (Online service)
Otros Autores: Gómez de Castro, Ana I. (Editor ), Wamsteker, Willem (Editor )
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Dordrecht : Springer Netherlands : Imprint: Springer, 2006.
Edición:1st ed. 2006.
Temas:
Acceso en línea:Texto Completo

MARC

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245 1 0 |a Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories  |h [electronic resource] /  |c edited by Ana I. Gómez de Castro, Willem Wamsteker. 
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505 0 |a Structure and Evolution of White Dwarfs and their Interaction with the Local Interstellar Medium -- Key Problems in Cool-Star Astrophysics -- UV Capabilities to Probe the Formation of Planetary Systems: From the ISM to Planets -- Ultraviolet Studies of Interacting Binaries -- The Need for Ultraviolet to Understand the Chemical Evolution of the Universe, and Cosmology -- Starbursts at Space Ultraviolet Wavelengths -- A View to the Future: Ultraviolet Studies of the Solar System -- Active Galaxies in the UV -- Fundamental Problems in Astrophysics -- Guidelines for Future UV Observatories -- Massive stars in the UV. 
520 |a Modern astrophysics is a mature science that has evolved from its early phase of discovery and classification to a physics-oriented discipline focused in finding answers to fundamental problems ranging from cosmology to the origin and diversity of life-sustainable systems in the Universe. For this very reason, progress of modern astrophysics requires the access to the electromagnetic spectrum in the broadest energy range. The Ultraviolet is a fundamental energy domain since it is one of the most powerful tool to study plasmas at temperatures in the 3,000-300,000~K range as well as electronic transitions of the most abundant molecules in the Universe. Moreover, the UV radiation field is a powerful astrochemical and photoionizing agent. This book describes the fundamental problems in modern astrophysics that cannot progress without easy and wide-spread access to modern UV instrumentation. 
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