Cited by 35Astrophysical Phenomena and ObservationsGalaxies: Formation, Evolution, PhenomenaAstrophysics and Cosmic Phenomena

Mapping Outflowing Gas in the Fermi Bubbles: A UV Absorption Survey of the Galactic Nuclear Wind*

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Ashley, Trisha, Fox, Andrew J., Jenkins, Edward B., Wakker, Bart P., Bordoloi, Rongmon, Lockman, Felix J., Savage, Blair D., Karim, Tanveer·2020·The Astrophysical Journal

Abstract

Using new ultraviolet (UV) spectra of five background quasars from the Cosmic Origins Spectrograph on the Hubble Space Telescope, we analyze the low-latitude ( ) regions of the Fermi Bubbles, the giant gamma-ray-emitting lobes at the Galactic Center. We combine these data with previous UV and atomic hydrogen (H i) data sets to build a comprehensive picture of the kinematics and metal column densities of the cool outflowing clouds entrained in the Fermi Bubbles. We find that the number of UV absorption components per sight line decreases as a function of increasing latitude, suggesting that the outflowing clouds become less common with increasing latitude. The Fermi Bubble H i clouds are accelerated up to b ∼ 7°, whereas when we model the UV Fermi Bubbles clouds’ deprojected flow velocities, we find that they are flat or even accelerating with distance from the Galactic center. This trend, which holds in both the northern and southern hemispheres, indicates that the nuclear outflow accelerates clouds throughout the Fermi Bubbles or has an acceleration phase followed by a coasting phase. Finally, we note the existence of several blueshifted high-velocity clouds at latitudes exceeding ∼30°, whose velocities cannot be explained by gas clouds confined to the inside of the gamma-ray-defined Fermi Bubbles. These anomalous-velocity clouds are likely in front of the Fermi Bubbles and could be remnants from past nuclear outflows. Overall, these observations form a valuable set of empirical data on the properties of cool gas in nuclear winds from star-forming galaxies.

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  1. Wakker, B. P., & van Woerden, H. 1997, ARA&A, 35, 217 · DOI

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Authors
Ashley, T., Fox, A. J., Jenkins, E. B., Wakker, B. P., Bordoloi, R., Lockman, F. J., Savage, B. D., & Karim, T.
Affiliations
  • Space Telescope Science Institute (US)
  • Princeton University (US)
  • University of Wisconsin–Madison (US)
  • North Carolina State University (US)
  • Center for Astrophysics Harvard & Smithsonian (US)
Venue
The Astrophysical Journal
Published
2020-07-31
Volume
898
Issue
2
Pages
128
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W3036996721
Cited by
35
References
47
Citations by year
2026: 5 · 2025: 3 · 2024: 4 · 2023: 5 · 2022: 12 · 2021: 4 · 2020: 2
FWCI
2.56
Type
journal article
Language
en
Open access
Locations
  • The Astrophysical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Funders
Space Telescope Science Institute (15339)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
Keywords
Fermi bubbles, gas outflows, UV absorption, quasar absorption lines, gas kinematics, high-velocity clouds, Galactic Center

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