Автор: Struve Otto Название: Stellar Evolution: An Exploration from the Observatory ISBN: 069162741X ISBN-13(EAN): 9780691627410 Издательство: Wiley Рейтинг: Цена: 7603.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание:
The sum of centuries of speculation on the probable course of evolution in stars is discussed by one of the world s greatest astronomers, with a full report of his own conclusions, How long stars exist, the relation of their luminosity to their mass, the evolution of a star in relation to the main sequence, the significance of rotation, are among the crucial problems considered. While the discussion is replete with technical detail, sufficient background is included to enable the amateur astronomer or anyone with scientific training to follow the argument.
Originally published in 1950.
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Автор: Leblanc, Francis Название: An introduction to stellar astrophysics ISBN: 0470699566 ISBN-13(EAN): 9780470699560 Издательство: Wiley Рейтинг: Цена: 7278.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Fundamental to our understanding of the universe, stellar astrophysics deals with observations, theoretical understanding, classification, computer simulations and modeling of stars and their evolution.
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.
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