A Search for Molecular Gas in the Nucleus of M87 and Implications for the Fueling of Supermassive Black Holes
Feedback under the microscope-II. Heating, gas uplift and mixing in the nearest cluster core
FUV line emission, gas kinematics, and discovery of Fe XXI l1354.1 in the sightline toward a filament in M87
Narrowband HST Images of M87: Evidence for a Disk of Ionized Gas around a Massive Black Hole
Star-forming accretion flows and the low-luminosity nuclei of giant elliptical galaxies
The M87 Black Hole Mass from Gas-dynamical Models of Space Telescope Imaging Spectrograph Observations
The Narrow-Line Regions of LINERS as Resolved with the Hubble Space Telescope
The Nature of Filamentary Cold Gas in the Core of the Virgo Cluster
The nature of nuclear Ha emission in LINERs
The Structure of Narrow-Line Region in LINERs
Velocity Profile of the Ionized Disk and the Mass of the Black Hole in M87
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-02-26T19:10:17Z/1994-02-26T22:25:57Z
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 et al., 1995, 'M87'S JET, NUCLEUS, AND HOT CORONA (FOS NO. 12): CYCLE 4 OBSERVATIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-yknr8ev
