Gas Accretion onto Galaxies

  • Andrew Fox
  • Romeel Davé

Part of the Astrophysics and Space Science Library book series (ASSL, volume 430)

Table of contents

  1. Front Matter
    Pages i-xix
  2. Philipp Richter
    Pages 15-47
  3. Felix J. Lockman
    Pages 49-65
  4. Jorge Sánchez Almeida
    Pages 67-94
  5. Nicolas Lehner
    Pages 117-144
  6. Glenn G. Kacprzak
    Pages 145-165
  7. Hsiao-Wen Chen
    Pages 167-194
  8. Sebastiano Cantalupo
    Pages 195-220
  9. Kyle R. Stewart
    Pages 249-270
  10. Filippo Fraternali
    Pages 323-353
  11. Back Matter
    Pages 369-373

About this book

Introduction

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.

Keywords

Accretion in Galaxies Accretion Models in Astrophysics Galactic Scale Accretion Gas Behavior in Galaxies Gas Inflow and Outflow in Galaxies Models of Accretion Observations of Accretion galaxy formation

Editors and affiliations

  • Andrew Fox
    • 1
  • Romeel Davé
    • 2
  1. 1.Space Telescope Science InstituteBaltimoreUSA
  2. 2.University of the Western CapeCape TownSouth Africa

Bibliographic information

  • DOI https://doi.org/10.1007/978-3-319-52512-9
  • Copyright Information Springer International Publishing AG 2017
  • Publisher Name Springer, Cham
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-3-319-52511-2
  • Online ISBN 978-3-319-52512-9
  • Series Print ISSN 0067-0057
  • Series Online ISSN 2214-7985
  • About this book
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