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Gas accretion onto galaxies

Dave, Romeel.

Gas accretion onto galaxies

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Gas accretion onto galaxiesedited by Andrew Fox, Romeel Dave.
其他作者:	Fox, Andrew.
出版者:	Cham :Springer International Publishing :2017.
面頁冊數:	xix, 373 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Planetary science.
標題:	Solar system.
電子資源:	http://dx.doi.org/10.1007/978-3-319-52512-9
ISBN:	9783319525129$q(electronic bk.)

Gas accretion onto galaxies
Gas accretion onto galaxies[electronic resource] /edited by Andrew Fox, Romeel Dave. - Cham :Springer International Publishing :2017. - xix, 373 p. :ill., digital ;24 cm. - Astrophysics and space science library,4300067-0057 ;. - Astrophysics and space science library ;379..

1.An Introduction to Gas Accretion onto Galaxies -- 2.Gas Accretion onto the Milky Way -- 3.Neutral Gas Accretion onto Nearby Galaxies -- 4.Gas Accretion and Star Formation Rates -- 5.Gas Accretion Traced in Absorption in Galaxy Spectroscopy -- 6.Gas Accretion via Lyman Limit Systems -- 7.Gas Accretion in Star-Forming Galaxies -- 8.The Circumgalactic Medium in Massive Halos -- 9.Gas Accretion and Giant Lya Nebulae -- 10.Gas Accretion and Galactic Chemical Evolution: Theory and Observations -- 11.Gas Accretion and Angular Momentum -- 12.Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations -- 13.The Effect of Galactic Feedback on Gas Accretion and Wind Recycling -- 14.Gas Accretion via Condensation and Fountains -- 15.Gas Accretion and Star-Formation Rates with IFUs and Background Quasars.

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 Milky Way in so-called High Velocity Clouds, but detecting accretion even around nearby galaxies has proved challenging; its multi-phase nature requires sensitive observations across the electromagnetic spectrum for full characterization. A promising approach involves looking for kinematic signatures, but accretion signatures are often confused with internal motions within galaxies. Accretion studies therefore touch a wide range of astrophysical processes, and hence a wide cross-section of the astronomical community. As observational facilities are finally able to access the wavelength ranges and depths at which accretion processes may be manifest, the time is right to survey these multiple lines of investigation and determine the state of the field in accretion studies of the baryon cycle.

ISBN: 9783319525129$q(electronic bk.)

Standard No.: 10.1007/978-3-319-52512-9doiSubjects--Topical Terms:

731409
Planetary science.
Subjects--Geographical Terms:

277832
Solar system.

LC Class. No.: QB601

Dewey Class. No.: 523.112

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505 0 $a 1.An Introduction to Gas Accretion onto Galaxies -- 2.Gas Accretion onto the Milky Way -- 3.Neutral Gas Accretion onto Nearby Galaxies -- 4.Gas Accretion and Star Formation Rates -- 5.Gas Accretion Traced in Absorption in Galaxy Spectroscopy -- 6.Gas Accretion via Lyman Limit Systems -- 7.Gas Accretion in Star-Forming Galaxies -- 8.The Circumgalactic Medium in Massive Halos -- 9.Gas Accretion and Giant Lya Nebulae -- 10.Gas Accretion and Galactic Chemical Evolution: Theory and Observations -- 11.Gas Accretion and Angular Momentum -- 12.Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations -- 13.The Effect of Galactic Feedback on Gas Accretion and Wind Recycling -- 14.Gas Accretion via Condensation and Fountains -- 15.Gas Accretion and Star-Formation Rates with IFUs and Background Quasars.
520 $a 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 Milky Way in so-called High Velocity Clouds, but detecting accretion even around nearby galaxies has proved challenging; its multi-phase nature requires sensitive observations across the electromagnetic spectrum for full characterization. A promising approach involves looking for kinematic signatures, but accretion signatures are often confused with internal motions within galaxies. Accretion studies therefore touch a wide range of astrophysical processes, and hence a wide cross-section of the astronomical community. As observational facilities are finally able to access the wavelength ranges and depths at which accretion processes may be manifest, the time is right to survey these multiple lines of investigation and determine the state of the field in accretion studies of the baryon cycle.
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