找回密碼
 To register

QQ登錄

只需一步,快速開(kāi)始

掃一掃,訪問(wèn)微社區(qū)

打印 上一主題 下一主題

Titlebook: Gas Accretion onto Galaxies; Andrew Fox,Romeel Davé Book 2017 Springer International Publishing AG 2017 Accretion in Galaxies.Accretion Mo

[復(fù)制鏈接]
查看: 27421|回復(fù): 58
樓主
發(fā)表于 2025-3-21 19:53:16 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Gas Accretion onto Galaxies
編輯Andrew Fox,Romeel Davé
視頻videohttp://file.papertrans.cn/381/380724/380724.mp4
概述Includes contributions from leading accretion experts on both observational data and on computer models.Elaborates on the baryon cycle, one of the central questions in the 2010 Astronomy Decadal Surve
叢書(shū)名稱Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Gas Accretion onto Galaxies;  Andrew Fox,Romeel Davé Book 2017 Springer International Publishing AG 2017 Accretion in Galaxies.Accretion Mo
描述.This edited volume presents the current state of gas accretion studies from both observational and theoretical perspectives, and charts our progress towards answering the fundamental yet elusive question of how galaxies get their gas. Understanding how galaxies form and evolve has been a central focus in astronomy for over a century. These studies have accelerated in the new millennium, driven by two key advances: the establishment of a firm concordance cosmological model that provides the backbone on which galaxies form and grow, and the recognition that galaxies grow not in isolation but within a “cosmic ecosystem” that includes the vast reservoir of gas filling intergalactic space. This latter aspect in which galaxies continually exchange matter with the intergalactic medium via inflows and outflows has been dubbed the “baryon cycle”. The topic of this book is directly related to the baryon cycle, in particular its least well constrained aspect, namely gas accretion...Accretion is a rare area of astrophysics in which the basic theoretical predictions are established, but the observations have been as yet unable to verify the expectations. Accretion has long been seen around the
出版日期Book 2017
關(guān)鍵詞Accretion in Galaxies; Accretion Models in Astrophysics; Galactic Scale Accretion; Gas Behavior in Gala
版次1
doihttps://doi.org/10.1007/978-3-319-52512-9
isbn_softcover978-3-319-84920-1
isbn_ebook978-3-319-52512-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing AG 2017
The information of publication is updating

書(shū)目名稱Gas Accretion onto Galaxies影響因子(影響力)




書(shū)目名稱Gas Accretion onto Galaxies影響因子(影響力)學(xué)科排名




書(shū)目名稱Gas Accretion onto Galaxies網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Gas Accretion onto Galaxies網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Gas Accretion onto Galaxies被引頻次




書(shū)目名稱Gas Accretion onto Galaxies被引頻次學(xué)科排名




書(shū)目名稱Gas Accretion onto Galaxies年度引用




書(shū)目名稱Gas Accretion onto Galaxies年度引用學(xué)科排名




書(shū)目名稱Gas Accretion onto Galaxies讀者反饋




書(shū)目名稱Gas Accretion onto Galaxies讀者反饋學(xué)科排名




單選投票, 共有 1 人參與投票
 

1票 100.00%

Perfect with Aesthetics

 

0票 0.00%

Better Implies Difficulty

 

0票 0.00%

Good and Satisfactory

 

0票 0.00%

Adverse Performance

 

0票 0.00%

Disdainful Garbage

您所在的用戶組沒(méi)有投票權(quán)限
沙發(fā)
發(fā)表于 2025-3-21 21:40:07 | 只看該作者
0067-0057 of the central questions in the 2010 Astronomy Decadal Surve.This edited volume presents the current state of gas accretion studies from both observational and theoretical perspectives, and charts our progress towards answering the fundamental yet elusive question of how galaxies get their gas. Unde
板凳
發(fā)表于 2025-3-22 01:00:58 | 只看該作者
地板
發(fā)表于 2025-3-22 07:03:27 | 只看該作者
Multiregional Projection and Stable Growth,he most recent studies follows that the present-day gas accretion rate of the Milky Way is a few solar masses per year, which is sufficient to maintain the Galaxy’s star-formation rate at its current level.
5#
發(fā)表于 2025-3-22 11:25:51 | 只看該作者
6#
發(fā)表于 2025-3-22 14:08:58 | 只看該作者
7#
發(fā)表于 2025-3-22 20:14:13 | 只看該作者
8#
發(fā)表于 2025-3-22 23:26:06 | 只看該作者
Gas Accretion onto the Milky Way,he most recent studies follows that the present-day gas accretion rate of the Milky Way is a few solar masses per year, which is sufficient to maintain the Galaxy’s star-formation rate at its current level.
9#
發(fā)表于 2025-3-23 03:09:00 | 只看該作者
10#
發(fā)表于 2025-3-23 07:47:25 | 只看該作者
The Effect of Galactic Feedback on Gas Accretion and Wind Recycling,s than gas accreting for the first time. Quantitative conclusions, however, vary between studies, because the amount of wind recycling is dependent on the details of the feedback model. We discuss these differences, known caveats, and ways to make progress in understanding how galaxies are fed at low redshift.
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛(ài)論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評(píng) 投稿經(jīng)驗(yàn)總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-11 09:15
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
霍林郭勒市| 丰都县| 大方县| 会宁县| 介休市| 临夏县| 湖北省| 阳春市| 特克斯县| 深泽县| 阜新市| 上饶县| 湖北省| 宝坻区| 伊通| 若尔盖县| 海兴县| 磴口县| 洞口县| 鄂托克前旗| 阿克苏市| 广宁县| 额尔古纳市| 宁乡县| 通州区| 河源市| 内江市| 中超| 吉林市| 大新县| 堆龙德庆县| 吴桥县| 襄垣县| 方山县| 呼玛县| 同江市| 卢湾区| 昔阳县| 铜川市| 济源市| 木兰县|