2013ApJ...765...27K
HST/COS Spectra of Three QSOs That Probe the Circumgalactic Medium of a Single Spiral Galaxy: Evidence for Gas Recycling and Outflow
Keeney, Brian A. ( Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, 389 UCB, Boulder, CO 80309, USA ); Stocke, John T. ( Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, 389 UCB, Boulder, CO 80309, USA ); Rosenberg, Jessica L. ( Department of Physics and Astronomy, George Mason University, Fairfax, VA 22030, USA ); Danforth, Charles W. ( Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, 389 UCB, Boulder, CO 80309, USA ); Ryan-Weber, Emma V. ( Centre for Astrophysics & Supercomputing, Swinburne University of Technology, Mail H30, P.O. Box 218, Hawthorn, 3122 VIC, Australia ); Shull, J. Michael ( Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, 389 UCB, Boulder, CO 80309, USA ); Savage, Blair D. ( Department of Astronomy, University of Wisconsin-Madison, 5534 Sterling Hall, 475 North Charter Street, Madison, WI 53706, USA ); Green, James C. ( Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, 389 UCB, Boulder, CO 80309, USA ) show affiliations
The Astrophysical Journal, Volume 765, Issue 1, article id. 27, 17 pp. (2013).
Published in Mar 2013
We have used the Cosmic Origins Spectrograph (COS) to obtain far-UV spectra of three closely spaced QSO sight lines that probe the circumgalactic medium (CGM) of an edge-on spiral galaxy, ESO 157-49, at impact parameters of 74 and 93 h -1 70 kpc near its major axis and 172 h -1 70 kpc along its minor axis. H I Lyα absorption is detected at the galaxy redshift in the spectra of all three QSOs, and metal lines of Si III, Si IV, and C IV are detected along the two major-axis sight lines. Photoionization models of these clouds suggest metallicities close to the galaxy metallicity, cloud sizes of ~1 kpc, and gas masses of ~104 M . Given the high covering factor of these clouds, ESO 157-49 could harbor ~2 × 109 M of warm CGM gas. We detect no metals in the sight line that probes the galaxy along its minor axis, but gas at the galaxy metallicity would not have detectable metal absorption with ionization conditions similar to the major-axis clouds. The kinematics of the major-axis clouds favor these being portions of a "galactic fountain" of recycled gas, while two of the three minor-axis clouds are constrained geometrically to be outflowing gas. In addition, one of our QSO sight lines probes a second more distant spiral, ESO 157-50, along its major axis at an impact parameter of 88 h -1 70 kpc. Strong H I Lyα and C IV absorption only are detected in the QSO spectrum at the redshift of ESO 157-50.Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Associated Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.
Keywords:
Free Keywords: Astrophysics - Cosmology and Extragalactic Astrophysics; galaxies: halos; galaxies: individual: ESO 157-49 ESO 157-50; intergalactic medium; quasars: absorption lines; quasars: individual: RX J0439.6─5311 HE 0439─5254 HE 0435─5304
Astronomy: galaxies: halos; galaxies: individual: ESO 157-49 ESO 157-50; intergalactic medium; quasars: absorption lines; quasars: individual: RX J0439.6─5311 HE 0439─5254 HE 0435─5304
arXiv: Astrophysics - Cosmology and Extragalactic Astrophysics
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