ALMA Observations of Atomic Carbon C I ( 3 P 1 - 3 P 0 ) and Low-J CO Lines in the Starburst Galaxy NGC 1808
Black hole feeding and star formation in NGC 1808
Dense Molecular Gas in the Starburst Nucleus of NGC 1808
Embedded clusters in NGC 1808 central starburst. Near-infrared imaging and spectroscopy
Evolution of Molecular Clouds in the Superwind Galaxy NGC 1808 Probed by ALMA Observations
Gas Dynamics and Outflow in the Barred Starburst Galaxy NGC 1808 Revealed with ALMA
On the morphology of sigma-drop galaxies
Star formation and gas flows in the centre of the NUGA galaxy NGC 1808 observed with SINFONI
The Connection between Bar Strength and Circumnuclear Dust Structure
The detection of stellar velocity dispersion drops in the central regions of five isolated Seyfert spirals
Three-Dimensional Integral Field Observations of 10 Galactic Winds. I. Extended Phase (gsim10 Myr) of Mass/Energy Injection Before the Wind Blows
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1997-08-14T23:03:13Z/1997-08-14T23:47:13Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Flood et al., 1998, 'Morphology of the active nucleus and radial filaments of NGC 1808', 1.0, European Space Agency, https://doi.org/10.5270/esa-1394tk1