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Titlebook: Multiwavelength Mapping of Galaxy Formation and Evolution; Proceedings of the E Alvio Renzini,Ralf Bender Conference proceedings 2005 Sprin

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書目名稱Multiwavelength Mapping of Galaxy Formation and Evolution
副標題Proceedings of the E
編輯Alvio Renzini,Ralf Bender
視頻videohttp://file.papertrans.cn/642/641354/641354.mp4
概述Includes supplementary material:
叢書名稱ESO Astrophysics Symposia
圖書封面Titlebook: Multiwavelength Mapping of Galaxy Formation and Evolution; Proceedings of the E Alvio Renzini,Ralf Bender Conference proceedings 2005 Sprin
描述.The possibilities of astronomical observation have dramatically increased over the last decade. Major satellites, like the Hubble Space Telescope, Chandra and XMM Newton, are complemented by numerous large ground-based observatories, from 8m-10m optical telescopes to sub-mm and radio facilities. As a result, observational astronomy has access to virtually the whole electromagnetic spectrum of galaxies, even at high redshifts. Theoretical models of galaxy formation and cosmological evolution now face a serious challenge to match the plethora of observational data...In October 2003, over 170 astronomers from 15 countries met for a 4-day workshop to extensively illustrate and discuss all major observational projects and ongoing theoretical efforts to model galaxy formation and evolution. This volume contains the complete proceedings of this meeting and is therefore a unique and timely overview of the current state of research in this rapidly evolving field..
出版日期Conference proceedings 2005
關鍵詞Astronomical Observation; Cosmology; Galaxy; Galaxy Clustering; Galaxy Evolution; Galaxy Formation; Observ
版次1
doihttps://doi.org/10.1007/b96746
isbn_softcover978-3-642-06509-5
isbn_ebook978-3-540-31641-1Series ISSN 1431-2433 Series E-ISSN 1611-6143
issn_series 1431-2433
copyrightSpringer-Verlag Berlin Heidelberg 2005
The information of publication is updating

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1431-2433 llites, like the Hubble Space Telescope, Chandra and XMM Newton, are complemented by numerous large ground-based observatories, from 8m-10m optical telescopes to sub-mm and radio facilities. As a result, observational astronomy has access to virtually the whole electromagnetic spectrum of galaxies,
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Multiwavelength Mapping of Galaxy Formation and Evolution978-3-540-31641-1Series ISSN 1431-2433 Series E-ISSN 1611-6143
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ESO Astrophysics Symposiahttp://image.papertrans.cn/n/image/641354.jpg
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https://doi.org/10.1007/b96746Astronomical Observation; Cosmology; Galaxy; Galaxy Clustering; Galaxy Evolution; Galaxy Formation; Observ
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Alvio Renzini,Ralf BenderIncludes supplementary material:
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