The Milky Way's kiloparsec-scale wind: A hybrid cosmic-ray and thermally driven outflow

John E. Everett*, Ellen G. Zweibel, Robert A. Benjamin, D. A N McCammon, Lindsay Rocks, John S. Gallagher

*Corresponding author for this work

Research output: Contribution to journalArticle

174 Scopus citations

Abstract

We apply a wind model, driven by combined cosmic-ray and thermal-gas pressure, to the Milky Way, and show that the observed Galactic diffuse soft X-ray emission can be better explained by a wind than by previous static gas models. We find that cosmic-ray pressure is essential to driving the observed wind. Having thus defined a "best-fit" model for a Galactic wind, we explore variations in the base parameters and show how the wind's properties vary with changes in gas pressure, cosmic-ray pressure, and density. We demonstrate the importance of cosmic rays in launching winds, and the effect cosmic rays have on wind dynamics. In addition, this model adds support to the hypothesis of Breitschwerdt and collaborators that such a wind may help to explain the relatively small gradient observed in γ-ray emission as a function of galactocentric radius.

Original languageEnglish (US)
Pages (from-to)258-270
Number of pages13
JournalAstrophysical Journal
Volume674
Issue number1
DOIs
StatePublished - Feb 10 2008

Keywords

  • Cosmic rays
  • Galaxy: evolution
  • ISM: jets and outflows
  • ISM: magnetic fields
  • X-rays: diffuse background

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Space and Planetary Science

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    Everett, J. E., Zweibel, E. G., Benjamin, R. A., McCammon, D. A. N., Rocks, L., & Gallagher, J. S. (2008). The Milky Way's kiloparsec-scale wind: A hybrid cosmic-ray and thermally driven outflow. Astrophysical Journal, 674(1), 258-270. https://doi.org/10.1086/524766