A Search for dense molecular gas in high redshift infrared-luminous galaxies
Sep, 20046 pages
Published in:
- Astrophys.J. 618 (2005) 586-591
e-Print:
- astro-ph/0409054 [astro-ph]
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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 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(H) cm). 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 QSO J1409+5628, with a velocity integrated line luminosity of K km s pc, while we obtain 3 upper limits to the HCN luminosity of the QSO J0751+2716 of K km s pc, K km s pc for the starburst galaxy J1401+0252, and K km s pc for the QSO J1148+5251. We compare the HCN data on these sources, plus three other high- 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 sources are within the scatter of the relationship between HCN and far-IR emission for low star-forming galaxies (truncated).- galaxies: active
- galaxies: formation
- galaxies: high-redshift
- galaxies: ISM
- galaxies: starburst
- infrared: galaxies
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