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Titlebook: Morphology, Kinematics and Star Formation Across the Hubble Sequence of Galaxies; Santiago Erroz-Ferrer Book 2016 Springer International P

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發(fā)表于 2025-3-21 17:37:01 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Morphology, Kinematics and Star Formation Across the Hubble Sequence of Galaxies
編輯Santiago Erroz-Ferrer
視頻videohttp://file.papertrans.cn/640/639439/639439.mp4
概述Nominated as an outstanding Ph.D. thesis by the University of La Laguna, Spain.Includes a thorough description of the methodology applied to study 3D kinematics.Contains important information not publ
叢書(shū)名稱Springer Theses
圖書(shū)封面Titlebook: Morphology, Kinematics and Star Formation Across the Hubble Sequence of Galaxies;  Santiago Erroz-Ferrer Book 2016 Springer International P
描述.This thesis discusses the evolution of galaxies through the study of the morphology, kinematics, and star formation properties of a sample of nearby galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS Fabry-Perot instrument on the William Herschel Telescope of a sample of 29 spiral galaxies. The work is closely related to the Spitzer Survey of Stellar Structure in Galaxies, and uses the mid-infrared data of that survey to determine key parameters of the galaxies studied. From these data, important results are obtained on streaming and other non-circular motions in galaxies, on the distribution and rates of star formation, and on how correlations of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies..
出版日期Book 2016
關(guān)鍵詞Morphology of galaxies; Kinematics of galaxies; Star Formation; galaxy evolution; Spiral Galaxies; Spitze
版次1
doihttps://doi.org/10.1007/978-3-319-26398-4
isbn_softcover978-3-319-38730-7
isbn_ebook978-3-319-26398-4Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing Switzerland 2016
The information of publication is updating

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發(fā)表于 2025-3-21 22:47:41 | 只看該作者
Morphology, Kinematics and Star Formation Across the Hubble Sequence of Galaxies978-3-319-26398-4Series ISSN 2190-5053 Series E-ISSN 2190-5061
板凳
發(fā)表于 2025-3-22 02:18:50 | 只看該作者
Santiago Erroz-FerrerNominated as an outstanding Ph.D. thesis by the University of La Laguna, Spain.Includes a thorough description of the methodology applied to study 3D kinematics.Contains important information not publ
地板
發(fā)表于 2025-3-22 08:07:51 | 只看該作者
Springer Theseshttp://image.papertrans.cn/m/image/639439.jpg
5#
發(fā)表于 2025-3-22 08:47:43 | 只看該作者
https://doi.org/10.1007/978-3-319-26398-4Morphology of galaxies; Kinematics of galaxies; Star Formation; galaxy evolution; Spiral Galaxies; Spitze
6#
發(fā)表于 2025-3-22 14:20:27 | 只看該作者
Morphology, Kinematics and Star Formation Across the Hubble Sequence of Galaxies
7#
發(fā)表于 2025-3-22 17:27:58 | 只看該作者
2190-5053 ons of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies..978-3-319-38730-7978-3-319-26398-4Series ISSN 2190-5053 Series E-ISSN 2190-5061
8#
發(fā)表于 2025-3-22 22:31:30 | 只看該作者
Book 2016galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS Fabry-Perot instrument on the William Herschel Telescope of a sample of 29 spiral galaxies. The work is closely related to the Spitzer Survey of Stellar Structure in Galaxies, and uses the mid-infrared data of
9#
發(fā)表于 2025-3-23 03:19:55 | 只看該作者
2190-5053 study 3D kinematics.Contains important information not publ.This thesis discusses the evolution of galaxies through the study of the morphology, kinematics, and star formation properties of a sample of nearby galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS
10#
發(fā)表于 2025-3-23 05:32:39 | 只看該作者
Book 2016motions in galaxies, on the distribution and rates of star formation, and on how correlations of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies..
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