Автор: Wilfried Boland; Hugo van Woerden Название: Birth and Evolution of Massive Stars and Stellar Groups ISBN: 9027721351 ISBN-13(EAN): 9789027721358 Издательство: Springer Рейтинг: Цена: 29209.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Proceedings of a Symposium held in Dwingeloo, The Netherlands, September 24-26, 1984 in honour of Adriaan Blaauw on the occasion of his 70th birthday
Описание: This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical foundations and numerical methods of such analyses.
Автор: V.E. Sherwood; L. Plaut Название: Variable Stars and Stellar Evolution ISBN: 902770578X ISBN-13(EAN): 9789027705785 Издательство: Springer Рейтинг: Цена: 60933.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Автор: D. Vanbeveren; W. van Rensbergen; C. de Loore Название: Evolution of Massive Stars ISBN: 9401044716 ISBN-13(EAN): 9789401044714 Издательство: Springer Рейтинг: Цена: 13974.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Автор: V.E. Sherwood; L. Plaut Название: Variable Stars and Stellar Evolution ISBN: 9027705798 ISBN-13(EAN): 9789027705792 Издательство: Springer Рейтинг: Цена: 60933.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Автор: Zdenek Kopal; J?rgen H. Rahe Название: Binary and Multiple Stars as Tracers of Stellar Evolution ISBN: 9400978634 ISBN-13(EAN): 9789400978638 Издательство: Springer Рейтинг: Цена: 12157.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Proceedings of the 69th Colloquium of the International Astronomical Union held in Bamberg, F.R.G., August 31-September 3, 1981
Описание: This book focuses on the stellar disk evolution and gas disk turbulence of the most numerous galaxies in the local Universe – the dwarf galaxies. The “outside-in” disk shrinking mode was established for a relatively large sample of dwarf galaxies for the first time, and this is in contrast to the “inside-out” disk growth mode found for spiral galaxies. Double exponential brightness profiles also correspond to double exponential stellar mass profiles for dwarf galaxies, which is again different from most spiral galaxies. The cool gas distribution in dwarf galaxies was probed with the spatial power spectra of hydrogen iodide (HI) gas emission, and provided indirect evidence that inner disks of dwarf galaxies have proportionally more cool gas than outer disks. The finding that no correlation exists between gas power spectral indices and star formation gave important constraints on the relation between turbulence and star formation in dwarf galaxies.
Автор: Ryan Название: Stellar Evolution and Nucleosynthesis ISBN: 0521133203 ISBN-13(EAN): 9780521133203 Издательство: Cambridge Academ Рейтинг: Цена: 8554.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This self-contained astrophysics textbook for advanced undergraduates explores how stars form, what happens to them as they age, and what becomes of them when they die. It contains a wealth of worked examples, exercises with full solutions, full colour illustrations, and clearly identified summaries, key facts and equations.
Автор: S. Kwok; Stuart R. Pottasch Название: Late Stages of Stellar Evolution ISBN: 9401081964 ISBN-13(EAN): 9789401081962 Издательство: Springer Рейтинг: Цена: 35218.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Over the last decade we have witnessed a rapid change in our understanding of the late stages of stellar evolution. A major stimulus to this has been the synthesis of observational data from different wavebands of the electromagnetic spectrum. The advent of infrared astronomy has led to the discovery of many luminous. late-type stars obscured by their circumstellar dust envelope. Sources discovered in the IRC and AFGL infrared sky surveys were followed up by radio observa- tions, leading to the widespread use of the OH and CO molecules as probes of the circumstellar envelopes. Advances in the technique of aperture synthesis have made possible observations with unprecedent resolving power, both in spectral-line and continuum. The success of the recent IRAS sky survey, with the detection of over 250,000 sources, brings the promise of even more exciting years ahead. This area of astronomical research is also blessed with the close collaboration between theorists and observers. New ideas are constantly being quantitatively tested by new data. Theoretical predictions are eagerly used as guides for further observations. This conference was initiated with the following objective: bring together workers in optical, infrared, radio and theoretical astronomy and let them confront each other. Based on the post-conference res- ponses we received, many of the participants have indeed found this Workshop a stimulating experience. The Workshop on the Late Stages of Stellar Evolution was held from 2-5 June 1986 in Calgary, Canada.
Описание: A stimulating introduction for undergraduates in astronomy, physics and applied mathematics, this second edition contains two new chapters and several new exercises. Clear and methodical, it explains processes in simple terms, while maintaining mathematical rigour, and leads students step-by-step to a global, comprehensive understanding of the subject.
Автор: Petit Название: Magnetic Fields throughout Stellar Evolution (IAU S302) ISBN: 1107044987 ISBN-13(EAN): 9781107044982 Издательство: Cambridge Academ Рейтинг: Цена: 13781.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: IAU Symposium 302 provides an overview of the emerging field of stellar magnetism. Covering all stages of stellar evolution, this volume features the most recent advances achieved by major observatories (ground-based and space-borne) and massively-parallel 3D numerical simulations, benefiting astronomers interested in the latest observational and theoretical developments.
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