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Significant primordial star formation at redshifts z ≈ 3–4

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  • Raul Jimenez

    (University of Pennsylvania)

  • Zoltan Haiman

    (Columbia University)

Abstract

Metal work Four recent anomalous results obtained during observation of high-redshift galaxies can be resolved at a stroke if a simple modification is made to the current models of galaxy formation. The modification is the assumption that 10–30% of the stars in many galaxies at redshifts of z = 3 to z = 4 are ‘primordial’. That is, they have not been enriched by metals — which to cosmologists means anything heavier than helium. Previously it had been assumed that micromixing of the heavier elements would have been extensive at the giga-year timescales implicit at these relatively low redshifts.

Suggested Citation

  • Raul Jimenez & Zoltan Haiman, 2006. "Significant primordial star formation at redshifts z ≈ 3–4," Nature, Nature, vol. 440(7083), pages 501-504, March.
  • Handle: RePEc:nat:nature:v:440:y:2006:i:7083:d:10.1038_nature04580
    DOI: 10.1038/nature04580
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