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Titlebook: Infrared Astronomy; Proceedings of the N Giancarlo Setti,Giovanni G. Fazio Conference proceedings 1978 D. Reidel Publishing Company, Dordre

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發(fā)表于 2025-3-21 18:36:50 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Infrared Astronomy
副標題Proceedings of the N
編輯Giancarlo Setti,Giovanni G. Fazio
視頻videohttp://file.papertrans.cn/467/466266/466266.mp4
叢書名稱Nato Science Series C:
圖書封面Titlebook: Infrared Astronomy; Proceedings of the N Giancarlo Setti,Giovanni G. Fazio Conference proceedings 1978 D. Reidel Publishing Company, Dordre
描述This volume contains a series of lectures presented at the 4th Course of the International School of Astrophysics, held in Erice (Sicily) from July 9 - July 20, 1977 at the "E. Majorana" Centre for Scientific Culture. The course was fully supported by a grant from the NATO Advanced Study Institute Programme. It was attended by 82 participants from 15 countries. Even though the infrared portion of the electromagnetic spectrum covers an extensive interval from the red region of the optical spectrum (10,000 A) to the microwave radio region (1 mm), its role in astronomy has been minimal until the last two decades. Until very recently, the only objects observed were the sun, the moon and the planets. A primary reason for this late development was the lack of sensitive detectors and the necessary cryogenic technology that must accompany their use. Recent progress in this technology has been paralleled by an ever increasing interest of astronomers in infrared observations, leading to a number of ex- tremely important results in different branches of astronomy. This becomes evident when one realizes that in many astrophysical conditions most of the energy is found to be channeled into the
出版日期Conference proceedings 1978
關鍵詞astronomy; astrophysics; interstellar matter; moon; planet; spectroscopy; star; star formation; stellar evol
版次1
doihttps://doi.org/10.1007/978-94-009-9815-5
isbn_softcover978-94-009-9817-9
isbn_ebook978-94-009-9815-5Series ISSN 1389-2185
issn_series 1389-2185
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1978
The information of publication is updating

書目名稱Infrared Astronomy影響因子(影響力)




書目名稱Infrared Astronomy影響因子(影響力)學科排名




書目名稱Infrared Astronomy網(wǎng)絡公開度




書目名稱Infrared Astronomy網(wǎng)絡公開度學科排名




書目名稱Infrared Astronomy被引頻次




書目名稱Infrared Astronomy被引頻次學科排名




書目名稱Infrared Astronomy年度引用




書目名稱Infrared Astronomy年度引用學科排名




書目名稱Infrared Astronomy讀者反饋




書目名稱Infrared Astronomy讀者反饋學科排名




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沙發(fā)
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https://doi.org/10.1007/978-94-009-9815-5astronomy; astrophysics; interstellar matter; moon; planet; spectroscopy; star; star formation; stellar evol
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Theoretical Aspects of the Infrared Emission from HII RegionsTreatment of the subject of IR emission from HII regions will necessitate considerable discussion of the parameters and properties of dust grains. Therefore I feel that I should first justify why and how dust problems are strictly related to the IR astronomy and also why they are interesting.
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Infrared Astronomical SpectroscopySpectroscopic instruments are designed to divide radiation into its component wavelengths (or frequencies) and to provide the observer with a display of this information at high signal-to-noise ratio (SNR).
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發(fā)表于 2025-3-23 07:47:32 | 只看該作者
ine think?? gestellt worden. Die erste offene Frage bei dieser insgesamt r?tselhaften Angelegenheit ist, wieso Turing sie überhaupt selbst so stellte, denn er wich ihr sofort aus und ersetzte sie durch eine andere, nicht minder dunkle, n?mlich die, ob sich eine menschliche Schiedsrichterin oder ein
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