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This volume presents the edited lecture notes of the First JETSET School on Jets from Young Stars: Models and Constraints, held by the Marie Curie Research and Training Network on JET Simulations, Experiments and Theory. The first half of the book is devoted to general observational constraints. The second section is devoted to theoretical knowledge of magneto-hydrodynamic processes pertinent to the jet launching mechanism in young stars.
Bruccoli Great War Collection at the University of South Carolina: An Illustrated Catalogue provides a reference tool for the study of one of the great watershed moments in history on both sides of the Atlantic serving historians, researchers, and collectors.
1 EAP and Study Skills: Definitions and Scope 2 Needs Analysis 3 Surveys: Students' Difficulties 4 EAP Syllabus and Course Design 5 Evaluation: Students and Courses 6 Learning Styles and Cultural Awareness 7 Methodology and Materials 8 Evaluating Materials 9 Academic Reading 10 Vocabulary Development 11 Academic Writing 12 Lectures and Note-Taking 13 Speaking for Academic Purposes 14 Reference/Research Skills 15 Examination Skills 16 Academic Discourse and Style 17 Subject-Specific Language 18 Materials Design and Production 19 Concerns and Research Appendices 1 Recommended Books and Journals 2 Educational Technology 3 Professional Associations and other Organisations 4 EAP Exams and Examining Bodies 5 ELT Publishers and Mail Order Firms (UK).
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This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, in degenerate stars (such as white dwarfs and neutron stars), exotic members called magnetars, and in their environments, as well as magnetic fields in the environments of black holes. These strong fields have a profound effect on the behavior of matter, visible in particular in highly variable processes like radiation in all known wavelengths, including Gamma-Ray bursts. The generation and structure of such strong magnetic fields and effects on the environment are also described.
It is over a quarter of a century since the discovery of out?ows from young stars. The intervening years have led to remarkable advances in our understanding of this phenomenon. Much of the progress can be attributed to advances in facilities and technologies, including not only larger telescopes but also improved instrument and detector performance. In addition protostellar out?ows have now been imaged from the ground and space at high spatial resolution, e. g. with HST, and at a wide - riety of wavelengths from X-rays to radio waves, revealing more and more about their physics. This veritable revolution in observation has been accompanied by an exponential growth in our ability to numerica...