標(biāo)題: Titlebook: Gas Accretion onto Galaxies; Andrew Fox,Romeel Davé Book 2017 Springer International Publishing AG 2017 Accretion in Galaxies.Accretion Mo [打印本頁] 作者: 充裕 時間: 2025-3-21 19:53
書目名稱Gas Accretion onto Galaxies影響因子(影響力)
作者: Malleable 時間: 2025-3-21 21:40
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作者: musicologist 時間: 2025-3-22 01:00 作者: doxazosin 時間: 2025-3-22 07:03
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.作者: Estrogen 時間: 2025-3-22 11:25 作者: 輕而薄 時間: 2025-3-22 14:08 作者: 輕而薄 時間: 2025-3-22 20:14 作者: 取之不竭 時間: 2025-3-22 23:26
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.作者: 慢跑 時間: 2025-3-23 03:09 作者: Anticonvulsants 時間: 2025-3-23 07:47
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.作者: 商品 時間: 2025-3-23 11:23
Gas Accretion and Star-Formation Rates with IFUs and Background Quasars,?3?.. or .?
作者: 心痛 時間: 2025-3-23 14:06 作者: mortuary 時間: 2025-3-23 21:10
Wolfgang Karl H?rdle,Léopold Simaretion is a challenging endeavor and we now have obtained a significant amount of observational evidence to support it. This chapter reviews the current observational evidence of gas accretion onto star-forming galaxies.作者: mucous-membrane 時間: 2025-3-23 22:47 作者: capillaries 時間: 2025-3-24 02:44 作者: Cumulus 時間: 2025-3-24 07:35
An Introduction to Gas Accretion onto Galaxies,primary sources of gas accretion are the intergalactic medium, satellite gas, and feedback material. There is support for each of these sources from observations and simulations, but the methods with which the fuel ultimately settles in to form stars remain murky.作者: Orthodontics 時間: 2025-3-24 14:12 作者: 思想靈活 時間: 2025-3-24 15:00 作者: filicide 時間: 2025-3-24 21:26 作者: 針葉類的樹 時間: 2025-3-25 00:11
Gas Accretion and Star Formation Rates,isks. Unfortunately, the observational support for this theoretical prediction is still indirect, and modeling and analysis are required to identify hints as actual signs of star formation feeding from metal-poor gas accretion. Thus, a meticulous interpretation of the observations is crucial, and th作者: 新鮮 時間: 2025-3-25 05:21
Gas Accretion Traced in Absorption in Galaxy Spectroscopy,oward the host system. Spectroscopy probing, e.g., Na?I resonance lines in the rest-frame optical or Mg?II and Fe?II in the near-ultraviolet is in principle sensitive to the infall of cool material at temperatures .?～?100–10,000?K anywhere along the line of sight to a galaxy’s stellar component. How作者: 愚笨 時間: 2025-3-25 09:28
Gas Accretion via Lyman Limit Systems,and out of galaxies through their circumgalactic medium (CGM). The overall low metallicity of the cold gaseous streams feeding galaxies seen in these simulations is the key to differentiating them from metal rich gas that is either outflowing or being recycled. In recent years, several groups have e作者: 無情 時間: 2025-3-25 15:41
Gas Accretion in Star-Forming Galaxies,stars over the lifetime of the Universe. Given its dramatic influence on a galaxy’s gas reservoir, gas accretion has to be largely responsible for how galaxies form and evolve. Therefore, given the importance of gas accretion, it is necessary to observe and quantify how these gas flows affect galaxy作者: kyphoplasty 時間: 2025-3-25 15:55
The Circumgalactic Medium in Massive Halos,the last decade, significant progress has been made in characterizing the cool circumgalactic gas in massive halos of ..?≈?10.?M. at intermediate redshifts using absorption spectroscopy. Systematic studies of halo gas around massive galaxies beyond the nearby universe are made possible by large spec作者: jovial 時間: 2025-3-25 22:47
Gas Accretion and Giant Ly, Nebulae,ding in some cases up to 500?kpc in size. In this chapter, I review the properties of the such nebulae discovered at .?>?2 and their connection with gas flows in and around galaxies and their halos. In particular, I show how current observations are used to constrain the physical properties and orig作者: 有節(jié)制 時間: 2025-3-26 02:47
Gas Accretion and Galactic Chemical Evolution: Theory and Observations,hasis is placed on the insights that result from using models to interpret observations. Even as the classical “G-dwarf problem” endures in the latest round of observational confirmation, a rich and tantalizing new phenomenology of relationships between .., ., SFR, and gas fraction is emerging both 作者: CARE 時間: 2025-3-26 06:26 作者: 教義 時間: 2025-3-26 09:03 作者: Flirtatious 時間: 2025-3-26 15:19
The Effect of Galactic Feedback on Gas Accretion and Wind Recycling,However, outflows driven by supernovae and active galactic nuclei not only eject gas from galaxies, but also prevent gas from accreting in the first place. Furthermore, gas previously ejected from a galaxy can re-accrete onto (the same or a different) galaxy. Because this gas has a high metallicity,作者: alliance 時間: 2025-3-26 17:08 作者: 提名 時間: 2025-3-27 00:48
Gas Accretion and Star-Formation Rates with IFUs and Background Quasars,show that their gas reservoir ought to be depleted in 0.5–2?Gyr. Thus, SFGs are thought to be fed by the continuous accretion of intergalactic gas in order to sustain their star-formation activity. However, direct observational evidence for this accretion phenomenon has been elusive. Theoretically, 作者: AGGER 時間: 2025-3-27 03:27
Book 2017 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作者: 密切關(guān)系 時間: 2025-3-27 05:31 作者: Rustproof 時間: 2025-3-27 12:03
Decomposition of Data Matrices by Factorse?II has provided evidence for ongoing gas accretion onto?>?5% of luminous, star-forming galaxies at .?～?0.?5–1. We then discuss the potentially ground-breaking benefits of future efforts to improve the spectral resolution of such studies, and to leverage spatially resolved spectroscopy for new cons作者: 思想流動 時間: 2025-3-27 14:43
Wolfgang Karl H?rdle,Léopold SimarLSs and LLSs so far studied are located in the CGM of galaxies with projected distances . 100–200?kpc. Regardless of the exact origin of the low-metallicity pLLSs/LLSs, there is a significant mass of cool, dense, low-metallicity gas in the CGM that may be available as fuel for continuing star format作者: Paleontology 時間: 2025-3-27 18:21 作者: 破譯密碼 時間: 2025-3-28 01:43 作者: 不可磨滅 時間: 2025-3-28 03:28
What Is Natural Language Processing?,rgers are an overall subdominant mechanism for delivering fresh gas to galaxies, but they trigger radial flows of previously accreted gas that flatten radial gas-phase metallicity gradients and temporarily suppress central metallicities. Radial gradients are generically expected to be steep at early作者: Fortuitous 時間: 2025-3-28 07:39
Complementary Libraries to TensorFlow 2.x,to the central galaxy. We discuss the implications of these simulations, reviewing a number of recent developments in the literature, and suggest a revision to the canonical model as it relates to the expected angular momentum content of gaseous halos around galaxies.作者: 收到 時間: 2025-3-28 12:45
Harald Niederreiter,Arne Winterhofer parts of discs and its efficiency drops for higher coronal temperatures. Thus galaxies are able to gather new gas as long as they do not become too massive nor fall into large halos and they maintain their star-forming gaseous discs.作者: 召集 時間: 2025-3-28 16:48
Gas Accretion and Star Formation Rates,l metallicity relationship, the relationship between disk morphology and gas metallicity, the existence of metallicity drops in starbursts of star-forming galaxies, the so-called G dwarf problem, the existence of a minimum metallicity for the star-forming gas in the local universe, the origin of the作者: AWRY 時間: 2025-3-28 18:58
Gas Accretion Traced in Absorption in Galaxy Spectroscopy,e?II has provided evidence for ongoing gas accretion onto?>?5% of luminous, star-forming galaxies at .?～?0.?5–1. We then discuss the potentially ground-breaking benefits of future efforts to improve the spectral resolution of such studies, and to leverage spatially resolved spectroscopy for new cons作者: Indicative 時間: 2025-3-29 00:17 作者: 外來 時間: 2025-3-29 04:55
The Circumgalactic Medium in Massive Halos,m massive quiescent galaxies. The origin of the gas closer in is currently less certain, but SNe Ia driven winds appear to contribute significantly to cool gas found at .?
作者: 柔聲地說 時間: 2025-3-29 07:28
Gas Accretion and Giant Ly, Nebulae,f massive galaxies. Spectroscopic studies suggest that, among the giant Ly. nebulae, the one associated with radio-loud AGN should have kinematics dominated by strong, ionized outflows within at least the inner 30–50?kpc. Radio-quiet nebulae instead present more quiescent kinematics compatible with 作者: 蔓藤圖飾 時間: 2025-3-29 14:57 作者: 人工制品 時間: 2025-3-29 18:11
Gas Accretion and Angular Momentum,to the central galaxy. We discuss the implications of these simulations, reviewing a number of recent developments in the literature, and suggest a revision to the canonical model as it relates to the expected angular momentum content of gaseous halos around galaxies.作者: 舉止粗野的人 時間: 2025-3-29 20:52 作者: AND 時間: 2025-3-30 00:16
0067-0057 retion 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 the978-3-319-84920-1978-3-319-52512-9Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 自傳 時間: 2025-3-30 04:33 作者: sleep-spindles 時間: 2025-3-30 09:39
Gas Accretion onto Galaxies978-3-319-52512-9Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 全國性 時間: 2025-3-30 14:30
Applied Multidimensional Systems Theory process and discuss the primary sources. The evidence for gas accretion includes the star formation rates and metallicities of galaxies, the evolution of the cold gas content of the universe with time, numerous indirect indicators for individual galaxies, and a few direct detections of inflow. The 作者: 哪有黃油 時間: 2025-3-30 16:54
Multiregional Projection and Stable Growth,disk. The corresponding gas-accretion rate represents a key parameter for the past, present, and future evolution of the Milky Way. In this chapter, we discuss our current understanding of gas accretion processes in the Galaxy by reviewing past and recent observational and theoretical studies. The f作者: A保存的 時間: 2025-3-30 20:44
https://doi.org/10.1007/978-1-4613-8740-4s scarce. Here we consider an inventory of starless gas “clouds” in and around galaxies of the Local Group to discern their general properties and see how they might appear in distant systems. The conclusion is that accreting gas without stars is detected almost entirely within the circumgalactic me作者: 起波瀾 時間: 2025-3-31 03:52
isks. Unfortunately, the observational support for this theoretical prediction is still indirect, and modeling and analysis are required to identify hints as actual signs of star formation feeding from metal-poor gas accretion. Thus, a meticulous interpretation of the observations is crucial, and th作者: Bereavement 時間: 2025-3-31 08:15 作者: Hyperplasia 時間: 2025-3-31 11:33 作者: 一個姐姐 時間: 2025-3-31 16:28
Wolfgang Karl H?rdle,Léopold Simarstars over the lifetime of the Universe. Given its dramatic influence on a galaxy’s gas reservoir, gas accretion has to be largely responsible for how galaxies form and evolve. Therefore, given the importance of gas accretion, it is necessary to observe and quantify how these gas flows affect galaxy作者: flourish 時間: 2025-3-31 20:40
https://doi.org/10.1007/978-3-662-05802-2the last decade, significant progress has been made in characterizing the cool circumgalactic gas in massive halos of ..?≈?10.?M. at intermediate redshifts using absorption spectroscopy. Systematic studies of halo gas around massive galaxies beyond the nearby universe are made possible by large spec
