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Windows on Galaxies - Proceedings of the Sixth Workshop of the Advanced School of Astronomy of the Ettore Majorana Centre for Scientific Culture, Erice, Italy, May 21-31, 1989 (Paperback, Softcover reprint of the original 1st ed. 1990)
Loot Price: R2,821
Discovery Miles 28 210
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Windows on Galaxies - Proceedings of the Sixth Workshop of the Advanced School of Astronomy of the Ettore Majorana Centre for Scientific Culture, Erice, Italy, May 21-31, 1989 (Paperback, Softcover reprint of the original 1st ed. 1990)
Series: Astrophysics and Space Science Library, 160
Expected to ship within 10 - 15 working days
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Along with the traditional optical window, many new windows have
been opened on galaxies in the last two decades, made possible by
new developments in groundbased detectors and by space missions
that allow detection of photons that are otherwise absorbed by the
Earth's atmosphere. Galaxies can now be observed in the radio,
submillimeter, IR, optical, UV, X- and gamma-ray bands, each window
allowing us to learn more about galactic components and properties.
These developments have also imposed the view that a deeper
understanding of even normal galaxies requires a panchromatic
approach, making use of all of the data gathered from the different
windows to synthesize a comprehensive physical image of these
complex astronomical systems. Windows on Galaxies presents a
comprehensive view of galaxies through all the available windows,
bringing together both theoretical and experimental approaches in
the form of a series of reviews reporting the most recent
developments complemented by contributed talks and discussions.
TEXT NO. 2 The sixth workshop of the Advanced School of Astronomy
examined galaxies through all available wavelength windows. Over
the last twenty years, new wavelength windows have been opened in
astronomy which have created many new possibilities for the
observation of the properties of galaxies. The outcome of the
meeting clearly stated that the approach towards the studying of
galaxies should be panchromatic. Each window, from radio to
gamma-rays, shows different components, and a synthesis of this
knowledge presents astronomers with a comprehensive physical image
of these astronomical systems: star formation, evolution of
galaxies, molecular contents, gas flows, interstellar matter and
properties of galaxies in the several wavelength fields are
discussed in this volume.
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