Intense star formation within resolved compact regions in a galaxy at z = 2.3

A.M. Swinbank, I. Smail, S. Longmore, A.I. Harris, A.J. Baker, C. De Breuck, J. Richard, A.C. Edge, R.J. Ivison, R. Blundell, Kristen Coppin, P. Cox, M. Gurwell, L.J. Hainline, M. Krips, A. Lundgren, R. Neri, B. Siana, G. Siringo, D.P. StarkD. Wilner, J.D. Younger

Research output: Contribution to journalLetterpeer-review

263 Citations (Scopus)
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Massive galaxies in the early Universe have been shown to be forming stars at surprisingly high rates. Prominent examples are dust-obscured galaxies which are luminous when observed at sub-millimetre wavelengths and which may be forming stars at a rate of 1,000 solar masses (M) per year. These intense bursts of star formation are believed to be driven by mergers between gas-rich galaxies. Probing the properties of individual star-forming regions within these galaxies, however, is beyond the spatial resolution and sensitivity of even the largest telescopes at present. Here we report observations of the sub-millimetre galaxy SMMJ2135-0102 at redshift z = 2.3259, which has been gravitationally magnified by a factor of 32 by a massive foreground galaxy cluster lens. This magnification, when combined with high-resolution sub-millimetre imaging, resolves the star-forming regions at a linear scale of only 100 parsecs. We find that the luminosity densities of these star-forming regions are comparable to the dense cores of giant molecular clouds in the local Universe, but they are about a hundred times larger and 10 7 times more luminous. Although vigorously star-forming, the underlying physics of the star-formation processes at z 2 appears to be similar to that seen in local galaxies, although the energetics are unlike anything found in the present-day Universe.
Original languageEnglish
Pages (from-to)733-736
Number of pages4
Issue number7289
Publication statusPublished - 1 Apr 2010


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