activity
20032009
most citedMolecular Gas in NUclei of GAlaxies (NUGA): IX. The decoupled bars and gas inflow in NGC 2782

109 citations · 581 across the 12 of their papers we have counts for

collaborators

17 papers

astro-ph.GA20096 cited

The Galactic Center: A Laboratory for Fundamental Astrophysics and Galactic Nuclei

A. Ghez, M. Morris, J. Lu +24

As the closest example of a galactic nucleus, the Galactic center presents an exquisite laboratory for learning about supermassive black holes (SMBH) and their environs. Detailed s…

astro-ph200847 cited

Multiplicity of young stars in and around R Corona Australis

R. Köhler, R. Neuhäuser, S. Krämer +3

The R CrA star-forming region has a small dark cloud with quite a number of protostars, T Tauri stars, and some Herbig Ae/Be stars, plus a number of weak-line T Tauri stars around…

astro-ph2008109 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-ph200843 cited

IRS 13N: a new comoving group of sources at the Galactic Center

K. Muzic, R. Schoedel, A. Eckart +2

Context: The Galactic Center IRS 13E cluster is located ~3.2'' from SgrA*. It is an extremely dense stellar association containing several Wolf-Rayet and O-type stars, at least fou…

astro-ph200730 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-ph200724 cited

Nuclear starburst-driven evolution of the central region in NGC 6764

S. Leon, A. Eckart, S. Laine +6

We study the CO and the radiocontinuum emission in an active galaxy to analyze the interplay between the central activity and the molecular gas. We present new high-resolution obse…