OUTFLOW VERSUS INFALL IN SPIRAL GALAXIES: METAL ABSORPTION IN THE HALO OF NGC 891 The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Bregman, Joel N., Eric D. Miller, Patrick Seitzer, C. R. Cowley, and Matthew J. Miller. “OUTFLOW VERSUS INFALL IN SPIRAL GALAXIES: METAL ABSORPTION IN THE HALO OF NGC 891.” The Astrophysical Journal 766, no. 1 (March 7, 2013): 57. © 2013 The American Astronomical Society As Published http://dx.doi.org/10.1088/0004-637x/766/1/57 Publisher IOP Publishing Version Final published version Citable link http://hdl.handle.net/1721.1/94577 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The Astrophysical Journal, 766:57 (6pp), 2013 March 20 doi:10.1088/0004-637X/766/1/57 C 2013. The American Astronomical Society. All rights reserved. Printed in the U.S.A. OUTFLOW VERSUS INFALL IN SPIRAL GALAXIES: METAL ABSORPTION IN THE HALO OF NGC 891 Joel N. Bregman1, Eric D. Miller2, Patrick Seitzer1,C.R.Cowley1, and Matthew J. Miller1 1 Department of Astronomy, University of Michigan, Ann Arbor, MI 48105, USA;
[email protected] 2 Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA Received 2010 July 8; accepted 2013 January 7; published 2013 March 7 ABSTRACT Gas accreting onto a galaxy will be of low metallicity while halo gas due to a galactic fountain will be of near-solar metallicity.