Titlebook: Historisches Erzählen und Lernen; Historische, theoret Martin Buchsteiner,Martin Nitsche Book 2016 Springer Fachmedien Wiesbaden 2016 Gesch

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书目名称Historisches Erzählen und Lernen影响因子(影响力)




书目名称Historisches Erzählen und Lernen影响因子(影响力)学科排名




书目名称Historisches Erzählen und Lernen网络公开度




书目名称Historisches Erzählen und Lernen网络公开度学科排名




书目名称Historisches Erzählen und Lernen被引频次




书目名称Historisches Erzählen und Lernen被引频次学科排名




书目名称Historisches Erzählen und Lernen年度引用




书目名称Historisches Erzählen und Lernen年度引用学科排名




书目名称Historisches Erzählen und Lernen读者反馈




书目名称Historisches Erzählen und Lernen读者反馈学科排名

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Martin Nitsche,Martin Buchsteinerfacility will be available to all levels of experimenters — be they from small laboratories or large organisations — through the 1980s. A summary description of the Space Shuttle and Spacelab programmes is provided, to help the future user in the fields covered by this book, to better appreciate the

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Bodo von Borrieselatively weak component between 0.1 MK and 1 MK, (b) a dominant component somewhere between 2 MK and 10 MK, and (c) in all cases but one a component in the formal solution at temperatures exceeding ≈ 20 MK. Where this hot tail is not associated with a real hot component, it is a spurious result ref

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Martin Nitscherophysics.Includes discussions on the goals and the expected.This book discusses the state of the art of the basic theoretical and observational topics related to black hole astrophysics. It covers all the main topics in this wide field, from the theory of accretion disks and formation mechanisms of

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Martin Buchsteinerr transiting exoplanets three fundamental atmospheric measurements are possible: transmission spectra—where atmospheric absorption features are detected across an exoplanets limb during transit, emission spectra—where the day-side average emission of the planet is detected during secondary eclipse e

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Sven Güntherl means of expanding on this information is by spectroscopic study of atmospheres. To do this requires a knowledge of the spectroscopy of the molecules, present or likely to be present, in their atmosphere which in turn demands access to the extensive laboratory data that characterises these species

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