The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3

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Abstract

Stellar archaeology1 shows that massive elliptical galaxies formed rapidly about ten billion years ago with star-formation rates of above several hundred solar masses per year. Their progenitors are probably the submillimetre bright galaxies2 at redshifts z greater than 2. Although the mean molecular gas mass3 (5 × 1010 solar masses) of the submillimetre bright galaxies can explain the formation of typical elliptical galaxies, it is inadequate to form elliptical galaxies4 that already have stellar masses above 2 × 1011 solar masses at z ≈ 2. Here we report multi-wavelength high-resolution observations of a rare merger of two massive submillimetre bright galaxies at z = 2.3. The system is seen to be forming stars at a rate of 2,000 solar masses per year. The star-formation efficiency is an order of magnitude greater than that of normal galaxies, so the gas reservoir will be exhausted and star formation will be quenched in only around 200 million years. At a projected separation of 19 kiloparsecs, the two massive starbursts are about to merge and form a passive elliptical galaxy with a stellar mass of about 4 × 1011 solar masses. We conclude that gas-rich major galaxy mergers with intense star formation can form the most massive elliptical galaxies by z ≈ 1.5.

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Figure 1: Multi-wavelength view of HXMM01.
Figure 2: The infrared luminosity and stellar masses of submillimetre galaxies.
Figure 3: The gas mass and dynamical state of submillimetre galaxies.

Change history

  • 19 June 2013

    The x and y axis labels of Fig. 1b were corrected.

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Acknowledgements

Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. This research has made use of data from the HerMES project (http://hermes.sussex.ac.uk/). HerMES is a Herschel Key Programme using Guaranteed Time from the SPIRE instrument team, ESAC scientists and a mission scientist. SPIRE has been developed by a consortium of institutes led by Cardiff University (UK) and including the University of Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, the University of Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, the University of Sussex (UK); and Caltech/JPL, IPAC and the University of Colorado (USA). This development has been supported by the following national funding agencies: CSA (Canada); NAOC (China); CEA, CNES and CNRS (France); ASI (Italy); MCINN (Spain); SNSB (Sweden); STFC (UK); and NASA (USA). The data presented in this paper will be released through the HeDaM Database in Marseille at http://hedam.oamp.fr/HerMES.

Author information

H.F. and A.C. wrote the manuscript and led the project. C.F., R.J.I., D.A.R., M.G., R.S.B. and A.I.H. contributed significantly to the taking and analysis of the follow-up data with various instruments. All other co-authors of this paper contributed extensively and equally by their varied contributions to the HerMES project, planning of HerMES observations, analysis of HerMES data, and by commenting on this manuscript as part of an internal review process.

Correspondence to Hai Fu or Asantha Cooray.

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The authors declare no competing financial interests.

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This file contains Supplementary Text and Data, Supplementary Figures 1-9, Supplementary Tables 1-3, Acknowledgements and additional references. (PDF 951 kb)

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Fu, H., Cooray, A., Feruglio, C. et al. The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3. Nature 498, 338–341 (2013) doi:10.1038/nature12184

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