Molecular gas in QSO host galaxies

(2) Smithsonian Astrophysical Observatory; (3) NASA/Goddard Space Flight Center; A. Eckart (1); C. Straubmeier (1); Germany; J.G. Staguhn (3) ((1) University of Cologne; M. Krips (2); S. Fischer (1); Submillimeter Array; T. Bertram (1)

arxiv: astro-ph/0511434 · v1 · submitted 2005-11-15 · 🌌 astro-ph

Molecular gas in QSO host galaxies

T. Bertram (1) , A. Eckart (1) , M. Krips (2) , C. Straubmeier (1) , S. Fischer (1) , J.G. Staguhn (3) ((1) University of Cologne , Germany , (2) Smithsonian Astrophysical Observatory

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Submillimeter Array USA (3) NASA/Goddard Space Flight Center USA)

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keywords sigmasourcessurveycatalogueclearlydetecteddetectionsemission

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We present the results of a survey for CO line emission from a sample of nearby QSO hosts taken from the Hamburg/ESO survey (HES) and the Veron-Cetty and Veron quasar catalogue. From a total of 39 observed sources we clearly detected 5 objects with >10sigma signals (HE 0108-4743, HE 0224-2834, J035818.7-612407, HE 1029-1831, HE 2211-3903). Further 6 sources show marginal detections on the 2sigma level.

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Molecular gas in QSO host galaxies

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