A Search for dense molecular gas in high redshift infrared-luminous galaxies

Sep, 2004
6 pages
Published in:
  • Astrophys.J. 618 (2005) 586-591
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20042008201220162019024681012
Abstract: (arXiv)
We present a search for HCN emission from four high redshift far infrared (IR) luminous galaxies. Current data and models suggest that these high zz IR luminous galaxies represent a major starburst phase in the formation of spheroidal galaxies, although many of the sources also host luminous active galactic nuclei (AGN), such that a contribution to the dust heating by the AGN cannot be precluded. HCN emission is a star formation indicator, tracing dense molecular hydrogen gas within star-forming molecular clouds (n(H2_2) 105\sim 10^5 cm3^{-3}). HCN luminosity is linearly correlated with IR luminosity for low redshift galaxies, unlike CO emission which can also trace gas at much lower density. We report a marginal detection of HCN (1-0) emission from the z=2.5832z=2.5832 QSO J1409+5628, with a velocity integrated line luminosity of LHCN=6.7±2.2×109L_{\rm HCN}'=6.7\pm2.2 \times10^{9} K km s1^{-1} pc2^2, while we obtain 3σ\sigma upper limits to the HCN luminosity of the z=3.200z=3.200 QSO J0751+2716 of LHCN=1.0×109L_{\rm HCN}'=1.0\times10^{9} K km s1^{-1} pc2^2, LHCN=1.6×109L_{\rm HCN}'=1.6\times10^{9} K km s1^{-1} pc2^2 for the z=2.565z= 2.565 starburst galaxy J1401+0252, and LHCN=1.0×1010L_{\rm HCN}'=1.0\times10^{10} K km s1^{-1} pc2^2 for the z=6.42z = 6.42 QSO J1148+5251. We compare the HCN data on these sources, plus three other high-zz IR luminous galaxies, to observations of lower redshift star-forming galaxies. The values of the HCN/far-IR luminosity ratios (or limits) for all the high zz sources are within the scatter of the relationship between HCN and far-IR emission for low zz star-forming galaxies (truncated).
  • galaxies: active
  • galaxies: formation
  • galaxies: high-redshift
  • galaxies: ISM
  • galaxies: starburst
  • infrared: galaxies
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