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Titlebook: Demographics of the Cold Universe with ALMA; From Interstellar an Seiji Fujimoto Book 2021 Springer Nature Singapore Pte Ltd. 2021 Observat

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發(fā)表于 2025-3-21 18:50:34 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Demographics of the Cold Universe with ALMA
副標題From Interstellar an
編輯Seiji Fujimoto
視頻videohttp://file.papertrans.cn/266/265301/265301.mp4
概述Nominated as an outstanding Ph.D. thesis by the University of Tokyo, Japan.Discusses the largest ALMA dataset ever constructed.Describes the wide landscape of the Universe, from galaxy to cosmic struc
叢書名稱Springer Theses
圖書封面Titlebook: Demographics of the Cold Universe with ALMA; From Interstellar an Seiji Fujimoto Book 2021 Springer Nature Singapore Pte Ltd. 2021 Observat
描述.This book presents the cold side of the Universe illustrated by the rest-frame, far-infrared emission with Atacama Large Millimeter/submillimeter Array (ALMA). The author constructed the largest-ever ALMA sample and dataset, which enables them to identify very faint, rest-frame, far-infrared dust continuums as well as the carbon fine-structure line emission from distant galaxies that have been missed in previous surveys. The observational findings described in this book reveal for the first time where and how much of the star formation, traced by the rest-frame far-infrared emission, is ongoing, from inter-stellar and circum-galactic media to cosmic structures. Moreover, since some of the findings are unexpected and as such challenge the current galaxy formation models, the book provides exciting questions that should be addressed in the next decades..
出版日期Book 2021
關鍵詞Observations with ALMA; Galaxy Formation; Galaxy Evolution; High Redshift; Star-forming Galaxies in the
版次1
doihttps://doi.org/10.1007/978-981-16-4979-0
isbn_softcover978-981-16-4981-3
isbn_ebook978-981-16-4979-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer Nature Singapore Pte Ltd. 2021
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 21:49:27 | 只看該作者
https://doi.org/10.1007/978-3-642-10850-1ting the evolutional connection from the dusty star-forming to the quiescent galaxies. In the context of previous ALMA studies for the . measurements, this is the first challenge for the statistical study of the . properties in a systematic way.
板凳
發(fā)表于 2025-3-22 00:39:02 | 只看該作者
地板
發(fā)表于 2025-3-22 08:01:18 | 只看該作者
Interstellar Medium Scale I: Galaxy Size,ting the evolutional connection from the dusty star-forming to the quiescent galaxies. In the context of previous ALMA studies for the . measurements, this is the first challenge for the statistical study of the . properties in a systematic way.
5#
發(fā)表于 2025-3-22 10:37:49 | 只看該作者
Circumgalactic Medium Scale: Metal-Enriched Gas Halo,s faint satellite galaxies. Interestingly, the radial profile of the . halo is well consistent with that of the Lyman-alpha (Ly.) halo that is universally identified around . normal star-forming galaxies in the recent deep MUSE observations, indicative of the association between the . and Ly. halos.
6#
發(fā)表于 2025-3-22 15:26:30 | 只看該作者
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發(fā)表于 2025-3-22 20:55:59 | 只看該作者
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發(fā)表于 2025-3-23 00:29:22 | 只看該作者
9#
發(fā)表于 2025-3-23 01:33:45 | 只看該作者
DICOM Media: Files, Folders, and DICOMDIRsr study, we have constructed 1220 ALMA submm/mm source sample from 1643 ALMA maps, that are the largest ALMA sample and dataset so far obtained, by making full use of the archive as well as our original data. In this chapter, we describe the ALMA sample and dataset used for the analysis at each scale.
10#
發(fā)表于 2025-3-23 07:26:52 | 只看該作者
https://doi.org/10.1007/978-3-642-10850-1ALMA 1-mm map. Owing to the stacked, deep high-resolution ALMA map, we find that our sample has an average . and rest-frame FIR ., ., values of . kpc and 1.2 ± 0.2, respectively. Interestingly, we obtain the rest-frame optical . and . of . (.) and . kpc (> .), suggesting that the dusty disk-like structure is embedded in the larger stellar disk.
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