Compact Star Clusters in M81. I. Data from Hubble Space Telescope Wide Field Planetary Camera 2 Imaging
Compact Star Clusters in M81. II. Two Populations
Dissecting the Power Sources of Low-Luminosity Emission-Line Galaxy Nuclei via Comparison of HST-STIS and Ground-Based Spectra
Kinematics of the Broad-Line Region in M81
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
Optical spectroscopy of local type-1 AGN LINERs
Spatially Resolved Narrow-Line Region Kinematics in Active Galactic Nuclei
Star Cluster Candidates in M81
STIS Spectroscopy of the Central 10 Parsecs of M81: Evidence for a Massive Black Hole
The HST view of the broad line region in low luminosity AGN
The HST view of the innermost narrow line region
Instrument
STIS, STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
1999-07-14T17:03:50Z/1999-07-14T21:43:44Z
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, Ford comma Holland, 2006, 'Kinematics of the Halpha Nuclear Disk in M81: A Search for a MBH in the Nearest LINER', 1.0, European Space Agency, https://doi.org/10.5270/esa-mjbjfh3