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OverviewThe papers in this study cover a range of scenarios, from disk and envelope around young stellar objects and protostars through to more aged stars and highly-evolved objects which exhibit considerable mass loss features. Significant advances and developments in observing facilities, instrumentation, computing power and techniques are described, together with a variety of theories, suggestions, observations and models. The formation, composition, effects and evolution of the material surrounding a stellar environment are also included. Full Product DetailsAuthor: Graeme D. Watt , Peredur M. WilliamsPublisher: Kluwer Academic Publishers Imprint: Kluwer Academic Publishers Edition: Reprinted from Astrophysics an and Em> ed. Weight: 1.276kg ISBN: 9780792335399ISBN 10: 0792335392 Pages: 636 Publication Date: July 1995 Audience: College/higher education , Professional and scholarly , Undergraduate , Postgraduate, Research & Scholarly Format: Hardback Publisher's Status: Active Availability: Out of stock ![]() The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available. Table of ContentsProtostellar and PMS shells and disks; PMS outflows; high mass stars and ultracompact HII regions; dust and gas - composition and chemistry; chemical evolution of circumstellar matter surrounding YSOs; late evolutionary stages of high mass stars; AGB stars, PPNe, and PNe; shocks in circumstellar winds; main sequence disks.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |