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Titlebook: Galactic and Extra-Galactic Radio Astronomy; Gerrit L. Verschuur,Kenneth I. Kellermann Book 19741st edition Springer-Verlag New York Inc.

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書目名稱Galactic and Extra-Galactic Radio Astronomy
編輯Gerrit L. Verschuur,Kenneth I. Kellermann
視頻videohttp://file.papertrans.cn/381/380336/380336.mp4
圖書封面Titlebook: Galactic and Extra-Galactic Radio Astronomy;  Gerrit L. Verschuur,Kenneth I. Kellermann Book 19741st edition Springer-Verlag New York Inc.
描述The present set of chapters by members of the staff of the National Radio Astronomy Observatory deals with the basic fields of research concerned with radio astronomy outside the solar system. The emphasis in this volume is on the type of data available and its interpretation. Basic theory is considered only where absolutely necessary, and little discussion of receivers or techniques is entered into in most of the chapters. The book is intended to take over where most textbooks on radio astronomy leave off, that is, in the discussion of what is actually known from the research done. In addition there is a chapter on the technical aspects of inter- ferometry and aperture synthesis, since so much of modern radio astronomy depends, and will depend in an ever increasing manner, on such tools. The editors want to stress that the chapters were not necessarily expected to be compre- hensive reviews of any of the fields being covered, but rather, overall outlines which the in- dividual authors feIt would be suitable for graduate students and interested workers in other fields. As a result, the lists of references are not complete. This only refiects the preferences of the individual author
出版日期Book 19741st edition
關鍵詞Galactic Radio Astronomy; Milchstrasse; Radio Astronomy; Radioastronomie; astronomy
版次1
doihttps://doi.org/10.1007/978-3-642-96178-6
isbn_softcover978-3-642-96180-9
isbn_ebook978-3-642-96178-6
copyrightSpringer-Verlag New York Inc. 1974
The information of publication is updating

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The Radio Characteristics of HII Regions and the Diffuse Thermal Background,d before the 19th century. Historically, objects of this type were called . (Latin for “clouds”) and were the subject of considerable speculation then as they are today. Careful observation with improved telescopes separated these objects into six distinct types : ., the nearest of which can frequen
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Pulsars,stronomy of recent years. The very unusual properties of these objects generated a great deal of effort on the part of both observational and theoretical astronomers. This resulted in the production of large amounts of observational data and numerous theories attempting to explain the observed prope
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The Galactic Magnetic Field,ctic supernova remnants, pulsars, and neutral hydrogen clouds, as well as observations of the non-thermal galactic background radiation, give information about the magnetic fields in interstellar space. This information is complemented by data on the optical polarization of starlight. Since rigorous
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