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

作者: 乳缽    時間: 2025-3-21 17:39
書目名稱Galactic and Extra-Galactic Radio Astronomy影響因子(影響力)




書目名稱Galactic and Extra-Galactic Radio Astronomy影響因子(影響力)學科排名




書目名稱Galactic and Extra-Galactic Radio Astronomy網(wǎng)絡公開度




書目名稱Galactic and Extra-Galactic Radio Astronomy網(wǎng)絡公開度學科排名




書目名稱Galactic and Extra-Galactic Radio Astronomy被引頻次




書目名稱Galactic and Extra-Galactic Radio Astronomy被引頻次學科排名




書目名稱Galactic and Extra-Galactic Radio Astronomy年度引用




書目名稱Galactic and Extra-Galactic Radio Astronomy年度引用學科排名




書目名稱Galactic and Extra-Galactic Radio Astronomy讀者反饋




書目名稱Galactic and Extra-Galactic Radio Astronomy讀者反饋學科排名





作者: 改變立場    時間: 2025-3-21 20:54

作者: –scent    時間: 2025-3-22 00:45
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
作者: 橢圓    時間: 2025-3-22 17:19
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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Galactic Nonthermal Continuum Emission,d through some process occurring at the subsolar point. These inferences were sharply revised when, after an entire year of observation, it was noted that the direction to the disturbance was not correlated with the position of the Sun, that it rather referred to afixed direction in space. Jansky (1
作者: HOWL    時間: 2025-3-24 00:12
The Radio Characteristics of HII Regions and the Diffuse Thermal Background,s. Because it is hotter than the surrounding medium, the gas of planetary and bright diffuse nebulae as well as supernova remnants emits spectral lines which appear in emission. These nebulae are categorically known as ..
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作者: 你不公正    時間: 2025-3-24 07:10
Pulsars,the Molonglo Radio Observatory in Australia, where about 30 of the presently known pulsars have been discovered. Pulsars were not discovered earlier because in most radio astronomical observations, receivers have relatively long time constants to smooth out random noise fluctuations. Consequently th
作者: 文件夾    時間: 2025-3-24 11:15
The Galactic Magnetic Field, medium, which contains both thermal electrons and magnetic fields, can be decomposed into two oppositely circularly polarized components having different phase velocities. On emergence from the medium the waves can be recombined, but with relative phases which may be different from those which they
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作者: Inkling    時間: 2025-3-24 20:35
Ernest H. Y. Chu,Sandra S. Powells. Because it is hotter than the surrounding medium, the gas of planetary and bright diffuse nebulae as well as supernova remnants emits spectral lines which appear in emission. These nebulae are categorically known as ..
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作者: 粗野    時間: 2025-3-25 08:52
https://doi.org/10.1007/978-1-4615-8261-8 medium, which contains both thermal electrons and magnetic fields, can be decomposed into two oppositely circularly polarized components having different phase velocities. On emergence from the medium the waves can be recombined, but with relative phases which may be different from those which they
作者: Synthesize    時間: 2025-3-25 14:08
Book 19741st editioniews 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
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Radio Galaxies and Quasars,1 minute, it was concluded that the discrete sources were galactic stars located at relatively small distances from our solar system. Thus the term “radio star” was often used in referring to these sources.
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作者: 用樹皮    時間: 2025-3-26 11:58
https://doi.org/10.1007/978-1-4684-5958-6n chronological order of detection the presently known interstellar molecules at radio wavelengths. In addition, CH, CH. , and CN have been detected at optical wavelengths, and H. and CO have been detected at UV wavelengths.
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作者: 痛苦一生    時間: 2025-3-27 21:44
Interstellar Neutral Hydrogen and its Small-Scale Structure,be an observable transition was made by van de Hulst in 1944 well before receivers existed to make the measurements, and in 1951 two groups reported the detection of emission from interstellar neutral hydrogen (HI) in the September 1 issue of . (Ewen and Purcell, 1951 ; and Muller and Oort, 1951).
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作者: esoteric    時間: 2025-3-28 02:37
Book 19741st edition 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 t
作者: 浮雕寶石    時間: 2025-3-28 07:32
https://doi.org/10.1007/978-3-642-96178-6Galactic Radio Astronomy; Milchstrasse; Radio Astronomy; Radioastronomie; astronomy
作者: 一加就噴出    時間: 2025-3-28 14:26
Bernard Dutrillaux,Jerome Lejeuneerable at 14.6-m wavelength and used this instrument to study local radio disturbances. He found that the static that was received usually could be categorized by one of the following descriptions: intermittent and strong, intermittent and weak, or very steady and weak. The first two types of static
作者: 雜色    時間: 2025-3-28 15:01

作者: HILAR    時間: 2025-3-28 20:03
Ernest H. Y. Chu,Sandra S. Powelld 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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作者: subordinate    時間: 2025-3-29 09:38

作者: originality    時間: 2025-3-29 15:09
https://doi.org/10.1007/978-1-4615-8261-8ctic 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
作者: buoyant    時間: 2025-3-29 15:36

作者: 貧窮地活    時間: 2025-3-29 22:38
https://doi.org/10.1007/978-1-4684-0958-1arge optical telescopes is limited to about a half arc second by atmospheric fluctuations, although the diffraction limit is much smaller. However, for radio frequencies a diffraction limit of about 1 arc minute at the highest radio frequencies is currently reached using filled-aperture telescopes.
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作者: 火光在搖曳    時間: 2025-3-30 11:53
https://doi.org/10.1007/978-1-4615-8303-5d their clusters, are used as sources of observational information, but cosmology must also provide the proper frame which enables their formation and evolution. The main emphasis in cosmology is mostly not on the objects. It is on the metric of space and time ; and on the average density of matter,
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