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Residual cooling and persistent star formation amid active galactic nucleus feedback in Abell 2597
dc.contributor.authorTremblay, G. R.en_US
dc.contributor.authorO’dea, C. P.en_US
dc.contributor.authorBaum, S. A.en_US
dc.contributor.authorClarke, T. E.en_US
dc.contributor.authorSarazin, C. L.en_US
dc.contributor.authorBregman, J. N.en_US
dc.contributor.authorCombes, F.en_US
dc.contributor.authorDonahue, M.en_US
dc.contributor.authorEdge, A. C.en_US
dc.contributor.authorFabian, A. C.en_US
dc.contributor.authorFerland, G. J.en_US
dc.contributor.authorMcNamara, B. R.en_US
dc.contributor.authorMittal, R.en_US
dc.contributor.authorOonk, J. B. R.en_US
dc.contributor.authorQuillen, A. C.en_US
dc.contributor.authorRussell, H. R.en_US
dc.contributor.authorSanders, J. S.en_US
dc.contributor.authorSalomé, P.en_US
dc.contributor.authorVoit, G. M.en_US
dc.contributor.authorWilman, R. J.en_US
dc.contributor.authorWise, M. W.en_US
dc.date.accessioned2012-08-09T14:56:11Z
dc.date.available2013-10-01T17:06:32Zen_US
dc.date.issued2012-08-01en_US
dc.identifier.citationTremblay, G. R.; O’dea, C. P. ; Baum, S. A.; Clarke, T. E.; Sarazin, C. L.; Bregman, J. N.; Combes, F.; Donahue, M.; Edge, A. C.; Fabian, A. C.; Ferland, G. J.; McNamara, B. R.; Mittal, R.; Oonk, J. B. R.; Quillen, A. C.; Russell, H. R.; Sanders, J. S.; Salomé, P. ; Voit, G. M.; Wilman, R. J.; Wise, M. W. (2012). "Residual cooling and persistent star formation amid active galactic nucleus feedback in Abell 2597." Monthly Notices of the Royal Astronomical Society 424(2). <http://hdl.handle.net/2027.42/92417>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/92417
dc.description.abstractNew Chandra X‐ray and Herschel Far‐Infrared (FIR) observations enable a multiwavelength study of active galactic nucleus (AGN) heating and intracluster medium (ICM) cooling in the brightest cluster galaxy (BCG) of Abell 2597 ( z = 0.0821). The new Chandra observations reveal the central ≲30 kpc X‐ray cavity network to be more extensive than previously thought, and associated with enough enthalpy to theoretically inhibit the inferred classical cooling flow. Nevertheless, we present new evidence, consistent with previous results, that a moderately strong residual cooling flow is persisting at 4–8 per cent of the classically predicted rates in a spatially structured manner amid the feedback‐driven excavation of the X‐ray cavity network. New Herschel observations are used to estimate warm and cold dust masses, a lower limit gas‐to‐dust ratio and a star formation rate consistent with previous measurements. [O  i ] and CO(2−1) line profiles are used to constrain the kinematics of the ∼10 9  M ⊙ reservoir of cold molecular gas. The cooling time profile of the ambient X‐ray atmosphere is used to map the locations of the observational star formation entropy threshold as well as the theoretical thermal instability threshold. Both lie just outside the ≲30‐kpc central region permeated by X‐ray cavities, and star formation as well as ionized and molecular gas lie interior to both. The young stars are distributed in an elongated region that is aligned with the radio lobes, and their estimated ages are both younger and older than the X‐ray cavity network, suggesting both jet‐triggered as well as persistent star formation over the current AGN feedback episode. Bright X‐ray knots that are coincident with extended Lyα and far‐ultraviolet continuum filaments motivate a discussion of structured cooling from the ambient hot atmosphere along a projected axis that is perpendicular to X‐ray cavity and radio axis. We conclude that the cooling ICM is the dominant contributor of the cold gas reservoir fuelling star formation and AGN activity in the Abell 2597 BCG.en_US
dc.publisherBlackwell Publishing Ltden_US
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherGalaxies: Activeen_US
dc.subject.otherGalaxies: Clusters: Generalen_US
dc.subject.otherGalaxies: Clusters: Individual: Abell 2597en_US
dc.subject.otherGalaxies: Clusters: Intracluster Mediumen_US
dc.subject.otherGalaxies: Star Formationen_US
dc.titleResidual cooling and persistent star formation amid active galactic nucleus feedback in Abell 2597en_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherEuropean Southern Observatory, Karl‐Schwarzschild‐Str. 2, 85748 Garching bei München, Germanyen_US
dc.contributor.affiliationotherDepartment of Physics, Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623, USAen_US
dc.contributor.affiliationotherChester F. Carlson Center for Imaging Science, 54 Lomb Memorial Drive, Rochester, NY 14623, USAen_US
dc.contributor.affiliationotherHarvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USAen_US
dc.contributor.affiliationotherRadcliffe Institute for Advanced Study, 10 Garden Street, Cambridge, MA 02138, USAen_US
dc.contributor.affiliationotherNaval Research Laboratory Remote Sensing Division, Code 7213 4555 Overlook Avenue SW, Washington, DC 20375, USAen_US
dc.contributor.affiliationotherDepartment of Astronomy, University of Virginia, PO Box 400325, Charlottesville, VA 22904‐4325, USAen_US
dc.contributor.affiliationotherObservatoire de Paris, LERMA, CNRS, 61 Av. de l’Observatoire, 75014 Paris, Franceen_US
dc.contributor.affiliationotherPhysics and Astronomy Department, Michigan State University, East Lansing, MI 48824‐2320, USAen_US
dc.contributor.affiliationotherDepartment of Physics, Durham University, Durham DH1 3LEen_US
dc.contributor.affiliationotherInstitute of Astronomy, Madingley Road, Cambridge CB3 0HAen_US
dc.contributor.affiliationotherDepartment of Physics, University of Kentucky, Lexington, KY 40506, USAen_US
dc.contributor.affiliationotherPhysics and Astronomy Department, Waterloo University, 200 University Avenue W., Waterloo, ON N2L 2G1, Canadaen_US
dc.contributor.affiliationotherASTRON, Netherlands Institute for Radio Astronomy, PO Box 2, 7990 AA Dwingeloo, the Netherlandsen_US
dc.contributor.affiliationotherDepartment of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/92417/1/j.1365-2966.2012.21278.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2012.21278.xen_US
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Remediation of Harmful Language

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