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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Beste egile batzuk: Goméz De Castro, Ana Inés (Argitalpenaren zuzendaria), Wamsteker, Willem, 1942- (Argitalpenaren zuzendaria)
Formatua: Livre numérique
Hizkuntza:Anglais
Argitaratua: Dordrecht : Springer Netherlands [20..].
Cham : Springer Nature
Edizioa:1st ed. 2006.
Sarrera elektronikoa:Accès sur la plateforme de l'éditeur
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Accès Université d'Orléans
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Oharra: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
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Edition sous un autre format:• Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories, Texte imprimé, 9789048172085
• Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories, Texte imprimé, 9789048108879
• Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories, Texte imprimé, 9781402048388
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505 1 |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. 
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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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