Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories
Editat de Ana I. Gómez de Castro, Willem Wamstekeren Limba Engleză Hardback – 9 oct 2006
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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Specificații
ISBN-13: 9781402048388
ISBN-10: 1402048386
Pagini: 176
Ilustrații: III, 170 p.
Dimensiuni: 210 x 279 x 13 mm
Greutate: 0.69 kg
Ediția:2006
Editura: SPRINGER NETHERLANDS
Colecția Springer
Locul publicării:Dordrecht, Netherlands
ISBN-10: 1402048386
Pagini: 176
Ilustrații: III, 170 p.
Dimensiuni: 210 x 279 x 13 mm
Greutate: 0.69 kg
Ediția:2006
Editura: SPRINGER NETHERLANDS
Colecția Springer
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
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.
Textul de pe ultima copertă
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.
This book describes the fundamental problems in modern astrophysics that cannot progress without easy and wide-spread access to modern UV instrumentation.
Caracteristici
Describes the fundamental problems in modern astrophysics that cannot progress without easy and wide-spread access to modern UV instrumentation