activity
19992026
most citedHigh molecular gas fractions in normal massive star forming galaxies in the young Universe

990 citations · 4.4k across the 42 of their papers we have counts for

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astro-ph2008★ 109 cited

Molecular Gas in NUclei of GAlaxies (NUGA): IX. The decoupled bars and gas inflow in NGC 2782

L. K. Hunt, F. Combes, S. García-Burillo +8

We present CO(1-0) and CO(2-1) maps of the starburst/Seyfert 1 galaxy NGC 2782, obtained with the IRAM interferometer. The CO emission is aligned along the stellar nuclear bar of r…

astro-ph2007★ 30 cited

Molecular gas in NUclei of GAlaxies (NUGA): VIII The Seyfert 2 NGC6574

E. Lindt-Krieg, A. Eckart, R. Neri +4

Within the frame of the NUclei of GAlaxies (NUGA) project, we have determined the distribution and kinematics of the molecular gas within the central kpc with high spatial resoluti…

astro-ph2007★ 50 cited

Molecular gas in NUclei of GAlaxies (NUGA) VII. NGC4569, a large scale bar funnelling gas into the nuclear region

F. Boone, A. J. Baker, E. Schinnerer +8

This work is part of the NUGA survey of CO emission in nearby active galaxies. We present observations of NGC4569, a member of the Virgo Cluster. We analyse the molecular gas distr…

astro-ph2007★ 62 cited

Molecular Gas in NUclei of GAlaxies (NUGA): VI. Detection of a molecular gas disk/torus via HCN in the Seyfert2 galaxy NGC6951?

M. Krips, R. Neri, S. Garcia-Burillo +8

Several studies of nearby active galaxies indicate significantly higher HCN-to-CO intensity ratios in AGN than in starburst (SB) environments. HCN enhancement can be caused by many…

astro-ph2007★ 48 cited

NUclei of GAlaxies: V. Radio emission in 7 NUGA sources

M. Krips, A. Eckart, T. P. Krichbaum +10

We present high angular resolution radio snap-shot observations of seven nearby low-luminosity active galaxies (LLAGN) from the NUclei of GAlaxies (NUGA) survey. The observations w…

astro-ph2006★ 55 cited

Detection of HNC and tentative detection of CN at z=3.9

M. Guelin, P. Salome, R. Neri +8

Molecular line emission from high-redshift galaxies holds great promise for the study of galaxy formation and evolution. The weak signals can only be detected with the largest mm-w…