AI Article Synopsis

  • Researchers trace molecular hydrogen using carbon monoxide (CO) emissions, with notable detections in quasars at redshifts greater than 2, including one at z = 4.69.
  • A new study reports CO emission from quasar SDSS J114816.64 + 525150.3, located at z = 6.42, indicating that heavy-element enrichment in molecular gas can occur quickly in young galaxies from the early Universe.

Article Abstract

Observations of molecular hydrogen in quasar host galaxies at high redshifts provide fundamental constraints on galaxy evolution, because it is out of this molecular gas that stars form. Molecular hydrogen is traced by emission from the carbon monoxide molecule, CO; cold H2 itself is generally not observable. Carbon monoxide has been detected in about ten quasar host galaxies with redshifts z > 2; the record-holder is at z = 4.69 (refs 1-3). Here we report CO emission from the quasar SDSS J114816.64 + 525150.3 (refs 5, 6) at z = 6.42. At that redshift, the Universe was only 1/16 of its present age, and the era of cosmic reionization was just ending. The presence of about 2 x 1010 M\circ of H2 in an object at this time demonstrates that molecular gas enriched with heavy elements can be generated rapidly in the youngest galaxies.

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http://dx.doi.org/10.1038/nature01821DOI Listing

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