CO(1-0) detection of molecular gas in the massive Spiderweb Galaxy (z = 2)

B. H.C. Emonts*, I. Feain, H. J.A. Röttgering, G. Miley, N. Seymour, R. P. Norris, C. L. Carilli, M. Villar-Martín, M. Y. Mao, E. M. Sadler, R. D. Ekers, G. A. van Moorsel, R. J. Ivison, L. Pentericci, C. N. Tadhunter, D. J. Saikia

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

The high-redshift radio galaxy MRC 1138-262 ('Spiderweb Galaxy'; z = 2.16) is one of the most massive systems in the early Universe and surrounded by a dense 'web' of proto-cluster galaxies. Using the Australia Telescope Compact Array, we detected CO(1-0) emission from cold molecular gas - the raw ingredient for star formation - across the Spiderweb Galaxy. We infer a molecular gas mass of MH2 = 6 × 1010 M· (for MH2/L 'CO = 0.8). While the bulk of the molecular gas coincides with the central radio galaxy, there are indications that a substantial fraction of this gas is associated with satellite galaxies or spread across the intergalactic medium on scales of tens of kpc. In addition, we tentatively detect CO(1-0) in the star-forming proto-cluster galaxy HAE 229, 250 kpc to the West. Our observations are consistent with the factthat the Spiderweb Galaxy is building up its stellar mass through a massive burst of widespread star formation. At maximum star formation efficiency, the molecular gas will be able to sustain the current star formation rate (SFR ≈ 1400 M· yr-1, S as traced by Seymour et al.) for about 40 Myr. This is similar to the estimated typical lifetime of a major starburst event in infrared luminous merger systems.

Original languageEnglish
Pages (from-to)3465-3471
Number of pages7
JournalMonthly Notices of the Royal Astronomical Society
Volume430
Issue number4
DOIs
Publication statusPublished - 1 Mar 2013

Keywords

  • Galaxies: active
  • Galaxies: clusters: individual: spiderweb
  • Galaxies: formation
  • Galaxies: high-redshift
  • Galaxies: individual: MRC 1138-262
  • Galaxies: ISM

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