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

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Gas Accretion onto Galaxies978-3-319-52512-9Series ISSN 0067-0057 Series E-ISSN 2214-7985

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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

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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

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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

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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

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Wolfgang Karl Härdle,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

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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