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Titlebook: Galactic and Extragalactic Infrared Spectroscopy; Proceedings of the X M. F. Kessler,J. P. Phillips Conference proceedings 1984 D. Reidel P

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發(fā)表于 2025-3-21 18:59:25 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy
副標(biāo)題Proceedings of the X
編輯M. F. Kessler,J. P. Phillips
視頻videohttp://file.papertrans.cn/381/380337/380337.mp4
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Galactic and Extragalactic Infrared Spectroscopy; Proceedings of the X M. F. Kessler,J. P. Phillips Conference proceedings 1984 D. Reidel P
描述The last major conference on infrared astronomy was the IAU Symposium No. 96 in June 1980. Since then, the discipline has continued to mature and to contribute to all branches of astrophysics. One particular area of growth has been in spectroscopic capabilities at all infrared wavelengths. The purpose of the Symposium in Toledo was to review the scientific questions to be addressed via infrared spectroscopy and to provide, in the proceedings, a useful summary of the field. The sensitivity of infrared spectroscopic observations is still generally limited by detector characteristics or by thermal background radiation. However in recent years improvements in detector technology together with developments in spectroscopic instrumentation have made possible both quite detailed spectroscopy of the brighter members of many classes of galactic sources and also begun to open up some infrared spectroscopy of extragalactic sources. The potential of the field in the next decade or two is clear. The lRAS mission has completed one of the pre-requisites, namely an all-sky photometric survey. Major space missions utilising cryogenic infrared telescopes have been approved in Europe (ISO) and seem l
出版日期Conference proceedings 1984
關(guān)鍵詞astronomy; galaxy; relativistic jet; spectroscopy; stars
版次1
doihttps://doi.org/10.1007/978-94-009-7251-3
isbn_softcover978-94-009-7253-7
isbn_ebook978-94-009-7251-3Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1984
The information of publication is updating

書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy影響因子(影響力)




書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy影響因子(影響力)學(xué)科排名




書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy被引頻次




書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy被引頻次學(xué)科排名




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書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy年度引用學(xué)科排名




書(shū)目名稱(chēng)Galactic and Extragalactic Infrared Spectroscopy讀者反饋




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Audrey D. Goddard,Ellen SolomonESA’s Space Science Department, which used to be called ESLAB, provides the study and project scientist for ESA’s scientific satellite programme. Each year this Department organizes an “ESLAB” symposium and it was decided that the 1982 symposium, held in Toledo, should be devoted to Galactic and Extragalactic Infrared Astronomy.
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https://doi.org/10.1007/978-1-4612-0371-1We consider atomic processes relevant to the interpretation of infrared measurements, with special emphasis on important, recent developments.
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Jennifer Li,David Greenwood,Mohamad KassemThe difficulties of making astronomical observations in the submillimeter spectrum are described in detail. Receiver technology and atmospheric absorption provide the biggest challenge. Techniques of overcoming these problems are discussed and some initial astronomical results are illustrated.
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Welcome AddressESA’s Space Science Department, which used to be called ESLAB, provides the study and project scientist for ESA’s scientific satellite programme. Each year this Department organizes an “ESLAB” symposium and it was decided that the 1982 symposium, held in Toledo, should be devoted to Galactic and Extragalactic Infrared Astronomy.
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