Is the current state of our Galaxy primarily the result of its initial conditions or is it the product of a lifetime of complex interactions with its environment? Gathered in this volume are papers presented at an international meeting in Granada, Spain, dedicated to exploring this fundamental question. This review examines all the key physical processes involved in the formation and evolution of the Milky Way. A dozen invited review articles by international experts summarise our understanding to date; whilst more than seventy topical research papers present the latest results. Together, these papers provide a view on topical issues such as disk instabilities, large-scale star formation, large-scale structure formation in our Galaxy, chemical evolution, Disk-Halo feedback, the galactic globular cluster system, stellar populations, and the formation of galaxies. Also included are three panel sessions identifying key routes for critical future research.
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Is the current state of our Galaxy primarily the result of its initial conditions or is it the product of a lifetime of complex interactions with its environment? Gathered in this volume are papers presented at an international meeting in Granada (Spain) dedicated to exploring this fundamental question. This timely review examines all the key physical processes involved in the formation and evolution of the Milky Way. A dozen invited review articles by international experts summarise our understanding to date; whilst more than 50 topical research papers present the latest results. Together, these papers provide a state-of-the-art view on topical issues such as disk instabilities, large-scale star formation, large-scale structure formation in our Galaxy, chemical evolution, disk-halo feedback, the galactic globular cluster system, stellar populations, and the formation of galaxies. Also included are three panel sessions identifying key routes for critical future research. For graduate students and researchers, this volume provides a valuable and pertinent review of our new vision of the formation and evolution of our Galaxy.
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Hardcover. Condition: Near Fine condition. NOT a library discard (illustrator). First Edition. Cambridge University Press, 1995. This is the 1995 HARDCOVER first edition. Near Fine condition. NO chips, tears, creases or fading. Bright and shiny. We have only this one copy, but it is available now and ready to ship today from Henderson, Nevada. Sharp corners. Square and tight. NO owner's name or bookplate. Small black mark on the top edge of the text block. Pages are otherwise crisp, clean and unmarked. NO underlining. NO highlighting. NO margin notes. Illustrations. Graphs. Tables, etc. Bound in the original mostly light blue pictorial boards. 7" wide by 10" tall. From the publisher: "Is the current state of our galaxy primarily the result of its initial conditions or is it the product of a lifetime of complex interactions with its environment? This volume presents papers dedicated to exploring this fundamental question and examines all the key physical processes involved in the formation and evolution of the Milky Way. A dozen invited review articles by international experts summarize our understanding to date while more than fifty topical research papers present the latest results. Together, these papers provide a state-of-the-art view of topical issues such as disk instabilities, large-scale star formation, large-scale structure formation in our galaxy, chemical evolution, disk-halo feedback, the galactic globular cluster system, stellar populations, and the formation of galaxies. Also included are three panel sessions identifying key routes for critical future research. For graduate students and researchers, this volume provides a valuable and timely review of our new vision of the formation and evolution of our galaxy.". First Edition. Hardcover. Near Fine condition/No dust jacket, as issued. Illus. by NOT a library discard. xvi, 360pp. Great Packaging, Fast Shipping. Seller Inventory # 032510
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