Further Evidence for a Supermassive Black Hole Mass-Pitch Angle Relation
Hubble Space Telescope Imaging of the Circinus Galaxy
Luminosity Models and Density Profiles for Nuclear Star Clusters for a Nearby Volume-limited Sample of 29 Galaxies
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Optical Counterparts of Ultraluminous X-Ray Sources Identified from Archival HST WFPC2 Images
Physical conditions of molecular gas in the Circinus galaxy Multi-J CO and Ci 3PP0 observations
Shocks, Seyferts, and the Supernova Remnant Connection: A Chandra Observation of the Circinus Galaxy
Supernova 1996cr: SN 1987As Wild Cousin?
The nuclear dust lane of Circinus: collimation without a torus
The warm molecular gas and dust of Seyfert galaxies: two different phases of accretion?
Unveiling the Central Parsec Region of an Active Galactic Nucleus: The Circinus Nucleus in the Near-Infrared with the Very Large Telescope
Updating the (supermassive black hole mass)-(spiral arm pitch angle) relation: a strong correlation for galaxies with pseudobulges
Instrument
NICMOS, NICMOS/NIC2, WFPC2, WFPC2/PC
Temporal Coverage
1998-05-07T21:21:32Z/1999-04-10T14:03:53Z
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, Wilson comma Andrew S., 2000, 'The Molecular Torus and Ionized Gas in the Circinus Galaxy', 1.0, European Space Agency, https://doi.org/10.5270/esa-lwaxiiq