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The optical/X-ray connection: intra-cluster medium iron content and galaxy optical luminosity in 20 galaxy clusters
dc.contributor.authorLaganá, T. F.en_US
dc.contributor.authorDupke, Renato A.en_US
dc.contributor.authorSodré Jr, L.en_US
dc.contributor.authorLima Neto, G. B.en_US
dc.contributor.authorDurret, F.en_US
dc.date.accessioned2010-06-01T20:53:46Z
dc.date.available2010-06-01T20:53:46Z
dc.date.issued2009-03-21en_US
dc.identifier.citationLaganÁ, T. F.; Dupke, R. A.; SodrÉ Jr, L.; Lima Neto, G. B.; Durret, F. (2009). "The optical/X-ray connection: intra-cluster medium iron content and galaxy optical luminosity in 20 galaxy clusters." Monthly Notices of the Royal Astronomical Society 394(1): 357-366. <http://hdl.handle.net/2027.42/73992>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/73992
dc.description.abstractX-ray observations of galaxy clusters have shown that the intra-cluster gas has iron abundances of about one-third of the solar value. These observations also show that part (if not all) of the intra-cluster gas metals was produced within the member galaxies. We present a systematic analysis of 20 galaxy clusters to explore the connection between the iron mass and the total luminosity of early- and late-type galaxies, and of the brightest cluster galaxies (BCGs). From our results, the intra-cluster medium (ICM) iron mass seems to correlate better with the luminosity of the BCGs than with that of the red and blue galaxy populations. As the BCGs cannot produce alone the observed amount of iron, we suggest that ram-pressure plus tidal stripping acts together to enhance, at the same time, the BCG luminosities and the iron mass in the ICM. Through the analysis of the iron yield, we have also estimated that SN Ia are responsible for more than 50 per cent of the total iron in the ICM. This result corroborates the fact that ram-pressure contributes to the gas removal from galaxies to the ICM, being very efficient for clusters in the temperature range 2 < kT (keV) < 10 .en_US
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dc.publisherBlackwell Publishing Ltden_US
dc.rightsJournal compilation © 2009 RASen_US
dc.subject.otherGalaxies: Clusters: Generalen_US
dc.subject.otherGalaxies: Evolutionen_US
dc.titleThe optical/X-ray connection: intra-cluster medium iron content and galaxy optical luminosity in 20 galaxy clustersen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI 48109-1090, USAen_US
dc.contributor.affiliationotherInstituto de Astronomia, GeofÍsica e C. Atmosf./USP, R. do MatÃo 1226, 05508-090. SÃo Paulo/SP, Brazilen_US
dc.contributor.affiliationotherInstitut d'Astrophysique de Paris, CNRS, UMR 7095, UniversitÉ Pierre et Marie Curie, 98bis Bd Arago, 75014 Paris, Franceen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/73992/1/j.1365-2966.2008.14285.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2008.14285.xen_US
dc.identifier.sourceMonthly Notices of the Royal Astronomical Societyen_US
dc.identifier.citedreferenceAdelman-McCarthy J. K. et al., 2007, ApJS, 172, 634en_US
dc.identifier.citedreferenceAllen S. W., Fabian A. C., 1998, MNRAS, 297, L63en_US
dc.identifier.citedreferenceAnders E., Grevesse N., 1989, Geochimica Cosmochimica Acta, 53, 197en_US
dc.identifier.citedreferenceArnaud M., Rothenflug R., Boulade O., Vigroux L., Vangioni-Flam E., 1992, A&A, 254, 49en_US
dc.identifier.citedreferenceBower R. G., Lucey J. R., Ellis R. S., 1992, MNRAS, 254, 601en_US
dc.identifier.citedreferenceBravo-Alfaro H., Cayatte V., van Gorkom J. H., Balkowski C., 2000, AJ, 119, 580en_US
dc.identifier.citedreferenceBrÜggen M., De Lucia G., 2008, MNRAS, 383, 1336en_US
dc.identifier.citedreferenceButcher H., Oemler A. Jr, 1984, ApJ, 285, L426en_US
dc.identifier.citedreferenceCypriano E. S., SodrÉ L. J., Campusano L. E., Dale D. A., Hardy E., 2006, AJ, 131, 2417en_US
dc.identifier.citedreferenceDavid L. P., Forman W., Jones C., 1990, ApJ, 359, 29en_US
dc.identifier.citedreferenceDavid L. P., Forman W., Jones C., 1991, ApJ, 380, 39en_US
dc.identifier.citedreferenceDe Grandi S., Ettori S., Longhetti M., Molendi S., 2004, A&A, 419, 7en_US
dc.identifier.citedreferenceDe Lucia G., Poggianti B. M., 2008, ASP Conf. Ser., 399, 314en_US
dc.identifier.citedreferenceDressler A., 1980, ApJ, 236, 351en_US
dc.identifier.citedreferenceDupke R. A., White R. E. III, 2000, ApJ, 528, 139en_US
dc.identifier.citedreferenceElbaz D., Arnaud M., Vangioni-Flam E., 1995, A&A, 303, 345en_US
dc.identifier.citedreferenceEttori S., 2005, MNRAS, 362, 110en_US
dc.identifier.citedreferenceFukugita M., Shimasaku K., Ichikawa T., 1995, PASP, 107, 945en_US
dc.identifier.citedreferenceGladders M. D., Lopez-Cruz O., Yee H. K. C., Kodama T., 1998, ApJ, 501, 571en_US
dc.identifier.citedreferenceGoto T., Yagi M., Tanaka M., Okamura S., 2004, MNRAS, 348, 515en_US
dc.identifier.citedreferenceGunn J. E., Gott J. R. I., 1972, ApJ, 176, 1en_US
dc.identifier.citedreferenceHaynes M. P., Giovanelli R., Chincarini G. L., 1984, ARA&A, 22, 445en_US
dc.identifier.citedreferenceHester J. A., 2006, ApJ, 647, 910en_US
dc.identifier.citedreferenceKantharia N. G., Ananthakrishnan S., Nityananda R., Hota A., 2005, A&A, 435, 483en_US
dc.identifier.citedreferenceKantharia N. G., Rao A. P., Sirothia S. K., 2008, MNRAS, 383, 173en_US
dc.identifier.citedreferenceKauffmann G. et al., 2003, MNRAS, 341, 33en_US
dc.identifier.citedreferenceLaganÁ T. F., Lima Neto G. B., Andrade-Santos F., Cypriano E. S., 2008, A&A, 485, 633en_US
dc.identifier.citedreferenceLevy L., Rose J. A., van Gorkom J. H., Chaboyer B., 2007, AJ, 133, 1104en_US
dc.identifier.citedreferenceMargoniner V. E., de Carvalho R. R., 2000, AJ, 119, 1562en_US
dc.identifier.citedreferenceMatteucci F., Gibson B. K., 1995, A&A, 304, 11en_US
dc.identifier.citedreferenceMaughan B. J., Jones C., Forman W., Van Speybroeck L., 2008, ApJS, 174, 117en_US
dc.identifier.citedreferenceMcCarthy I. G., Frenk C. S., Font A. S., Lacey C. G., Bower R. G., Mitchell N. L., Balogh M. L., Theuns T., 2008, MNRAS, 383, 593en_US
dc.identifier.citedreferenceMitchell R. J., Culhane J. L., Davison P. J. N., Ives J. C., 1976, MNRAS, 175, 29 pen_US
dc.identifier.citedreferenceMurante G., Giovalli M., Gerhard O., Arnaboldi M., Borgani S., Dolag K., 2007, MNRAS, 377, 2en_US
dc.identifier.citedreferenceMushotzky R. F., Loewenstein M., 1997, ApJ, 481, L63en_US
dc.identifier.citedreferenceMushotzky R., Loewenstein M., Arnaud K. A., Tamura T., Fukazawa Y., Matsushita K., Kikuchi K., Hatsukade I., 1996, ApJ, 466, 686en_US
dc.identifier.citedreferenceNomoto K., Iwamoto K., Nakasato N., Thielemann F.-K., Brachwitz F., Tsujimoto T., Kubo Y., Kishimoto N., 1997, Nucl. Phys. A, 621, 467en_US
dc.identifier.citedreferencePoggianti B. M., 1997, A&AS, 122, 399en_US
dc.identifier.citedreferencePress W. H., Teukolsky S. A., Vetterling W. T., Flannery B. P., 1992, Numerical Recipes in FORTRAN. The Art of Scientific Computing, 2nd edn. Cambridge Univ. Press, Cambridgeen_US
dc.identifier.citedreferenceRakos K. D., Schombert J. M., 1995, ApJ, 439, 47en_US
dc.identifier.citedreferenceRenzini A., Ciotti L., D'Ercole A., Pellegrini S., 1993, ApJ, 419, 52en_US
dc.identifier.citedreferenceRomeo A. D., Napolitano N. R., Covone G., Sommer-Larsen J., Antonuccio-Delogu V., Capaccioli M., 2008, MNRAS, 389, 13en_US
dc.identifier.citedreferenceSerlemitsos P. J., Smith B. W., Boldt E. A., Holt S. S., Swank J. H., 1977, ApJ, 211, L63en_US
dc.identifier.citedreferenceSodrÉ L. J., Capelato H. V., Steiner J. E., Mazure A., 1989, AJ, 97, 1279en_US
dc.identifier.citedreferenceSolanes J. M., Manrique A., GarcÍa-GÓmez C., GonzÁlez-Casado G., Giovanelli R., Haynes M. P., 2001, ApJ, 548, 97en_US
dc.identifier.citedreferenceSun M., Donahue M., Voit G. M., 2007, ApJ, 671, 190en_US
dc.identifier.citedreferenceThielemann F.-K., Hashimoto M.-A., Nomoto K., 1990, ApJ, 349, 222en_US
dc.identifier.citedreferenceTonnesen S., Bryan G. L., 2008, ApJ, 684, L9en_US
dc.identifier.citedreferenceToomre A., Toomre J., 1972, ApJ, 178, 623en_US
dc.identifier.citedreferenceTozzi P., Rosati P., Ettori S., Borgani S., Mainieri V., Norman C., 2003, ApJ, 593, 705en_US
dc.identifier.citedreferenceVikhlinin A., Kravtsov A., Forman W., Jones C., Markevitch M., Murray S. S., Van Speybroeck L., 2006, ApJ, 640, 691en_US
dc.identifier.citedreferenceVollmer B., Huchtmeier W., van Driel W., 2005, A&A, 439, 921en_US
dc.identifier.citedreferenceWhite R. E. III, 1991, ApJ, 367, 69en_US
dc.identifier.citedreferenceYork D. G. et al., 2000, AJ, 120, 1579en_US
dc.identifier.citedreferenceYoshii Y., Tsujimoto T., Nomoto K., 1996, ApJ, 462, 266en_US
dc.identifier.citedreferenceZhang Y.-Y., Finoguenov A., BÖhringer H., Kneib J.-P., Smith G. P., Czoske O., Soucail G., 2007, A&A, 467, 437en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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