A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies

M. McDonald; M. Bayliss; B. A. Benson; R. J. Foley; J. Ruel; P. Sullivan; S. Veilleux; K. A. Aird; M. L.N. Ashby; M. Bautz; G. Bazin; L. E. Bleem; M. Brodwin; J. E. Carlstrom; C. L. Chang; H. M. Cho; A. Clocchiatti; T. M. Crawford; A. T. Crites; T. De Haan; S. Desai; M. A. Dobbs; J. P. Dudley; E. Egami; W. R. Forman; G. P. Garmire; E. M. George; M. D. Gladders; A. H. Gonzalez; N. W. Halverson; N. L. Harrington; F. W. High; G. P. Holder; W. L. Holzapfel; S. Hoover; J. D. Hrubes; C. Jones; M. Joy; R. Keisler; L. Knox; A. T. Lee; E. M. Leitch; J. Liu; M. Lueker; D. Luong-Van; A. Mantz; D. P. Marrone; J. J. McMahon; J. Mehl; S. S. Meyer; E. D. Miller; L. Mocanu; J. J. Mohr; T. E. Montroy; S. S. Murray; T. Natoli; S. Padin; T. Plagge; C. Pryke; T. D. Rawle; C. L. Reichardt; A. Rest; M. Rex; J. E. Ruhl; B. R. Saliwanchik; A. Saro; J. T. Sayre; K. K. Schaffer; L. Shaw; E. Shirokoff; R. Simcoe; J. Song; H. G. Spieler; B. Stalder; Z. Staniszewski; A. A. Stark; K. Story; C. W. Stubbs; R. Šuhada; A. Van Engelen; K. Vanderlinde; J. D. Vieira; A. Vikhlinin; R. Williamson; O. Zahn; A. Zenteno

doi:10.1038/nature11379

A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies

M. McDonald, M. Bayliss, B. A. Benson, R. J. Foley, J. Ruel, P. Sullivan, S. Veilleux, K. A. Aird, M. L.N. Ashby, M. Bautz, G. Bazin, L. E. Bleem, M. Brodwin, J. E. Carlstrom, C. L. Chang, H. M. Cho, A. Clocchiatti, T. M. Crawford, A. T. Crites, T. De HaanS. Desai, M. A. Dobbs, J. P. Dudley, E. Egami, W. R. Forman, G. P. Garmire, E. M. George, M. D. Gladders, A. H. Gonzalez, N. W. Halverson, N. L. Harrington, F. W. High, G. P. Holder, W. L. Holzapfel, S. Hoover, J. D. Hrubes, C. Jones, M. Joy, R. Keisler, L. Knox, A. T. Lee, E. M. Leitch, J. Liu, M. Lueker, D. Luong-Van, A. Mantz, D. P. Marrone, J. J. McMahon, J. Mehl, S. S. Meyer, E. D. Miller, L. Mocanu, J. J. Mohr, T. E. Montroy, S. S. Murray, T. Natoli, S. Padin, T. Plagge, C. Pryke, T. D. Rawle, C. L. Reichardt, A. Rest, M. Rex, J. E. Ruhl, B. R. Saliwanchik, A. Saro, J. T. Sayre, K. K. Schaffer, L. Shaw, E. Shirokoff, R. Simcoe, J. Song, H. G. Spieler, B. Stalder, Z. Staniszewski, A. A. Stark, K. Story, C. W. Stubbs, R. Šuhada, A. Van Engelen, K. Vanderlinde, J. D. Vieira, A. Vikhlinin, R. Williamson, O. Zahn, A. Zenteno

Research output: Contribution to journal › Review article › peer-review

150 Scopus citations

Abstract

In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the clusters lifetime, leading to continuous cooling flows of gas sinking towards the cluster centre, yet no such cooling flow has been observed. The low observed star-formation rates and cool gas masses for these cool-core clusters suggest that much of the cooling must be offset by feedback to prevent the formation of a runaway cooling flow. Here we report X-ray, optical and infrared observations of the galaxy cluster SPT-CLJ2344-4243 (ref. 11) at redshift z = 0.596. These observations reveal an exceptionally luminous (8.2Ã-10 45 ergs-1) galaxy cluster that hosts an extremely strong cooling flow (around 3,820 solar masses a year). Further, the central galaxy in this cluster appears to be experiencing a massive starburst (formation of around 740 solar masses a year), which suggests that the feedback source responsible for preventing runaway cooling in nearby cool-core clusters may not yet be fully established in SPT-CLJ2344-4243. This large star-formation rate implies that a significant fraction of the stars in the central galaxy of this cluster may form through accretion of the intracluster medium, rather than (as is currently thought) assembling entirely via mergers.

Original language	English (US)
Pages (from-to)	349-352
Number of pages	4
Journal	Nature
Volume	488
Issue number	7411
DOIs	https://doi.org/10.1038/nature11379
State	Published - Aug 16 2012

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McDonald, M., Bayliss, M., Benson, B. A., Foley, R. J., Ruel, J., Sullivan, P., Veilleux, S., Aird, K. A., Ashby, M. L. N., Bautz, M., Bazin, G., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Chang, C. L., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., ... Zenteno, A. (2012). A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies. Nature, 488(7411), 349-352. https://doi.org/10.1038/nature11379

McDonald, M, Bayliss, M, Benson, BA, Foley, RJ, Ruel, J, Sullivan, P, Veilleux, S, Aird, KA, Ashby, MLN, Bautz, M, Bazin, G, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, De Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Egami, E, Forman, WR, Garmire, GP, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McMahon, JJ, Mehl, J, Meyer, SS, Miller, ED, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Natoli, T, Padin, S, Plagge, T, Pryke, C, Rawle, TD, Reichardt, CL, Rest, A, Rex, M, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Simcoe, R, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, Šuhada, R, Van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O & Zenteno, A 2012, 'A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies', Nature, vol. 488, no. 7411, pp. 349-352. https://doi.org/10.1038/nature11379

@article{7755da29495e4c54b15e6f5897bbba41,

title = "A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies",

abstract = "In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the clusters lifetime, leading to continuous cooling flows of gas sinking towards the cluster centre, yet no such cooling flow has been observed. The low observed star-formation rates and cool gas masses for these cool-core clusters suggest that much of the cooling must be offset by feedback to prevent the formation of a runaway cooling flow. Here we report X-ray, optical and infrared observations of the galaxy cluster SPT-CLJ2344-4243 (ref. 11) at redshift z = 0.596. These observations reveal an exceptionally luminous (8.2{\~A}-10 45 ergs-1) galaxy cluster that hosts an extremely strong cooling flow (around 3,820 solar masses a year). Further, the central galaxy in this cluster appears to be experiencing a massive starburst (formation of around 740 solar masses a year), which suggests that the feedback source responsible for preventing runaway cooling in nearby cool-core clusters may not yet be fully established in SPT-CLJ2344-4243. This large star-formation rate implies that a significant fraction of the stars in the central galaxy of this cluster may form through accretion of the intracluster medium, rather than (as is currently thought) assembling entirely via mergers.",

author = "M. McDonald and M. Bayliss and Benson, {B. A.} and Foley, {R. J.} and J. Ruel and P. Sullivan and S. Veilleux and Aird, {K. A.} and Ashby, {M. L.N.} and M. Bautz and G. Bazin and Bleem, {L. E.} and M. Brodwin and Carlstrom, {J. E.} and Chang, {C. L.} and Cho, {H. M.} and A. Clocchiatti and Crawford, {T. M.} and Crites, {A. T.} and {De Haan}, T. and S. Desai and Dobbs, {M. A.} and Dudley, {J. P.} and E. Egami and Forman, {W. R.} and Garmire, {G. P.} and George, {E. M.} and Gladders, {M. D.} and Gonzalez, {A. H.} and Halverson, {N. W.} and Harrington, {N. L.} and High, {F. W.} and Holder, {G. P.} and Holzapfel, {W. L.} and S. Hoover and Hrubes, {J. D.} and C. Jones and M. Joy and R. Keisler and L. Knox and Lee, {A. T.} and Leitch, {E. M.} and J. Liu and M. Lueker and D. Luong-Van and A. Mantz and Marrone, {D. P.} and McMahon, {J. J.} and J. Mehl and Meyer, {S. S.} and Miller, {E. D.} and L. Mocanu and Mohr, {J. J.} and Montroy, {T. E.} and Murray, {S. S.} and T. Natoli and S. Padin and T. Plagge and C. Pryke and Rawle, {T. D.} and Reichardt, {C. L.} and A. Rest and M. Rex and Ruhl, {J. E.} and Saliwanchik, {B. R.} and A. Saro and Sayre, {J. T.} and Schaffer, {K. K.} and L. Shaw and E. Shirokoff and R. Simcoe and J. Song and Spieler, {H. G.} and B. Stalder and Z. Staniszewski and Stark, {A. A.} and K. Story and Stubbs, {C. W.} and R. {\v S}uhada and {Van Engelen}, A. and K. Vanderlinde and Vieira, {J. D.} and A. Vikhlinin and R. Williamson and O. Zahn and A. Zenteno",

note = "Funding Information: Acknowledgements M.McD. was supported at MIT by NASA through the Chandra X-ray Observatory. The South Pole Telescope is supported by the National Science Foundation, with partial support provided by the Kavli Foundation, and the Moore Foundation. Support for X-ray analysis was provided by NASA. Work at McGill University is supported by NSERC, the CRC programme, and CIfAR, and at Harvard University by the NSF. S.V. acknowledges a Senior NPP Award held at the NASA Goddard Space Flight Center. R.K. acknowledges a NASA Hubble Fellowship, B.A.B. acknowledges a KICP Fellowship, M.A.D. acknowledges an Alfred P. Sloan Research Fellowship, and O.Z. acknowledges a BCCP fellowship.",

year = "2012",

month = aug,

day = "16",

doi = "10.1038/nature11379",

language = "English (US)",

volume = "488",

pages = "349--352",

journal = "Nature",

issn = "0028-0836",

publisher = "Nature Publishing Group",

number = "7411",

}

TY - JOUR

T1 - A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies

AU - McDonald, M.

AU - Bayliss, M.

AU - Benson, B. A.

AU - Foley, R. J.

AU - Ruel, J.

AU - Sullivan, P.

AU - Veilleux, S.

AU - Aird, K. A.

AU - Ashby, M. L.N.

AU - Bautz, M.

AU - Bazin, G.

AU - Bleem, L. E.

AU - Brodwin, M.

AU - Carlstrom, J. E.

AU - Chang, C. L.

AU - Cho, H. M.

AU - Clocchiatti, A.

AU - Crawford, T. M.

AU - Crites, A. T.

AU - De Haan, T.

AU - Desai, S.

AU - Dobbs, M. A.

AU - Dudley, J. P.

AU - Egami, E.

AU - Forman, W. R.

AU - Garmire, G. P.

AU - George, E. M.

AU - Gladders, M. D.

AU - Gonzalez, A. H.

AU - Halverson, N. W.

AU - Harrington, N. L.

AU - High, F. W.

AU - Holder, G. P.

AU - Holzapfel, W. L.

AU - Hoover, S.

AU - Hrubes, J. D.

AU - Jones, C.

AU - Joy, M.

AU - Keisler, R.

AU - Knox, L.

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Liu, J.

AU - Lueker, M.

AU - Luong-Van, D.

AU - Mantz, A.

AU - Marrone, D. P.

AU - McMahon, J. J.

AU - Mehl, J.

AU - Meyer, S. S.

AU - Miller, E. D.

AU - Mocanu, L.

AU - Mohr, J. J.

AU - Montroy, T. E.

AU - Murray, S. S.

AU - Natoli, T.

AU - Padin, S.

AU - Plagge, T.

AU - Pryke, C.

AU - Rawle, T. D.

AU - Reichardt, C. L.

AU - Rest, A.

AU - Rex, M.

AU - Ruhl, J. E.

AU - Saliwanchik, B. R.

AU - Saro, A.

AU - Sayre, J. T.

AU - Schaffer, K. K.

AU - Shaw, L.

AU - Shirokoff, E.

AU - Simcoe, R.

AU - Song, J.

AU - Spieler, H. G.

AU - Stalder, B.

AU - Staniszewski, Z.

AU - Stark, A. A.

AU - Story, K.

AU - Stubbs, C. W.

AU - Šuhada, R.

AU - Van Engelen, A.

AU - Vanderlinde, K.

AU - Vieira, J. D.

AU - Vikhlinin, A.

AU - Williamson, R.

AU - Zahn, O.

AU - Zenteno, A.

N1 - Funding Information: Acknowledgements M.McD. was supported at MIT by NASA through the Chandra X-ray Observatory. The South Pole Telescope is supported by the National Science Foundation, with partial support provided by the Kavli Foundation, and the Moore Foundation. Support for X-ray analysis was provided by NASA. Work at McGill University is supported by NSERC, the CRC programme, and CIfAR, and at Harvard University by the NSF. S.V. acknowledges a Senior NPP Award held at the NASA Goddard Space Flight Center. R.K. acknowledges a NASA Hubble Fellowship, B.A.B. acknowledges a KICP Fellowship, M.A.D. acknowledges an Alfred P. Sloan Research Fellowship, and O.Z. acknowledges a BCCP fellowship.

PY - 2012/8/16

Y1 - 2012/8/16

N2 - In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the clusters lifetime, leading to continuous cooling flows of gas sinking towards the cluster centre, yet no such cooling flow has been observed. The low observed star-formation rates and cool gas masses for these cool-core clusters suggest that much of the cooling must be offset by feedback to prevent the formation of a runaway cooling flow. Here we report X-ray, optical and infrared observations of the galaxy cluster SPT-CLJ2344-4243 (ref. 11) at redshift z = 0.596. These observations reveal an exceptionally luminous (8.2Ã-10 45 ergs-1) galaxy cluster that hosts an extremely strong cooling flow (around 3,820 solar masses a year). Further, the central galaxy in this cluster appears to be experiencing a massive starburst (formation of around 740 solar masses a year), which suggests that the feedback source responsible for preventing runaway cooling in nearby cool-core clusters may not yet be fully established in SPT-CLJ2344-4243. This large star-formation rate implies that a significant fraction of the stars in the central galaxy of this cluster may form through accretion of the intracluster medium, rather than (as is currently thought) assembling entirely via mergers.

AB - In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the clusters lifetime, leading to continuous cooling flows of gas sinking towards the cluster centre, yet no such cooling flow has been observed. The low observed star-formation rates and cool gas masses for these cool-core clusters suggest that much of the cooling must be offset by feedback to prevent the formation of a runaway cooling flow. Here we report X-ray, optical and infrared observations of the galaxy cluster SPT-CLJ2344-4243 (ref. 11) at redshift z = 0.596. These observations reveal an exceptionally luminous (8.2Ã-10 45 ergs-1) galaxy cluster that hosts an extremely strong cooling flow (around 3,820 solar masses a year). Further, the central galaxy in this cluster appears to be experiencing a massive starburst (formation of around 740 solar masses a year), which suggests that the feedback source responsible for preventing runaway cooling in nearby cool-core clusters may not yet be fully established in SPT-CLJ2344-4243. This large star-formation rate implies that a significant fraction of the stars in the central galaxy of this cluster may form through accretion of the intracluster medium, rather than (as is currently thought) assembling entirely via mergers.

UR - http://www.scopus.com/inward/record.url?scp=84865153365&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84865153365&partnerID=8YFLogxK

U2 - 10.1038/nature11379

DO - 10.1038/nature11379

M3 - Review article

C2 - 22895340

SN - 0028-0836

VL - 488

SP - 349

EP - 352

JO - Nature

JF - Nature

IS - 7411

ER -

A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies

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