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Titlebook: Water Snowline in Protoplanetary Disks; Shota Notsu Book 2020 The Editor(s) (if applicable) and The Author(s), under exclusive license to

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發(fā)表于 2025-3-21 16:10:00 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Water Snowline in Protoplanetary Disks
編輯Shota Notsu
視頻videohttp://file.papertrans.cn/1022/1021076/1021076.mp4
概述Nominated as an outstanding Ph.D. thesis by Kyoto University, Japan.Received Best Presentation Award at the Japanese Society for Planetary Sciences (JSPS) Autumn Meeting 2017.Proposes a new method to
叢書名稱Springer Theses
圖書封面Titlebook: Water Snowline in Protoplanetary Disks;  Shota Notsu Book 2020 The Editor(s) (if applicable) and The Author(s), under exclusive license to
描述.This book presents pioneering work on a critical observational test of the planet formation theory based on the theoretical study of the water snowline, beyond which water takes the form of ice, in the protoplanetary disks – the place where planets are formed. Since the water snowline is thought to divide the regions of rocky and gas-giant planet formation, the location of the snowline is essential for the planet formation process...The book proposes a novel method to locate the snowlines using high-dispersion spectroscopic observations of water vapor lines, which is based on in sophisticated chemical modeling and line radiative transfer calculations. The author obtained the water vapor distribution in the disks using the chemical reaction network, which includes photoreactions and gas–grain interactions. The simulated transition lines of water vapor in the disks demonstrate that relatively weak transition lines with moderate excitation energies are the best tracers of water snowline...Furthermore, the author observed submillimeter lines of water vapor in a disk using ALMA (Atacama Large Millimeter/submillimeter Array) to obtain the upper limit of the line fluxes with the highest
出版日期Book 2020
關鍵詞Molecules in Protoplanetary Disks; T Tauri Stars; Protoplanetary Disks; Chemical Evolution in a Disk Mi
版次1
doihttps://doi.org/10.1007/978-981-15-7439-9
isbn_softcover978-981-15-7441-2
isbn_ebook978-981-15-7439-9Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
The information of publication is updating

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Shota NotsuNominated as an outstanding Ph.D. thesis by Kyoto University, Japan.Received Best Presentation Award at the Japanese Society for Planetary Sciences (JSPS) Autumn Meeting 2017.Proposes a new method to
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2190-5053 ciences (JSPS) Autumn Meeting 2017.Proposes a new method to .This book presents pioneering work on a critical observational test of the planet formation theory based on the theoretical study of the water snowline, beyond which water takes the form of ice, in the protoplanetary disks – the place wher
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Introduction,wline in protoplanetary disks is important to understand the planetesimal and planet formation processes, and the water trail to rocky planets. The line profiles from disks are usually affected by doppler shift due to Keplerian rotation. Thus, the line profiles are sensitive to the radial distributi
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Modeling Studies I. The Case of the T Tauri Star,ated chemical structures of the disk using the self-consistent physical models of a typical T Tauri disk. We confirmed that the water gas abundance is high not only in the hot disk midplane within the . snowline, but also in the outer hot surface and photodesorption region. Next, we calculated the p
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發(fā)表于 2025-3-23 07:57:21 | 只看該作者
Modeling Studies I. The Case of the T Tauri Star,ated chemical structures of the disk using the self-consistent physical models of a typical T Tauri disk. We confirmed that the water gas abundance is high not only in the hot disk midplane within the . snowline, but also in the outer hot surface and photodesorption region. Next, we calculated the p
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