A Kinematic Model for the Narrow-Line Region in NGC 4151
Feedback from Mass Outflows in Nearby Active Galactic Nuclei. II. Outflows in the Narrow-line Region of NGC 4151
Gas Cloud Kinematics near the Nucleus of NGC 4151
High-Velocity Line Emission in the Narrow-Line Region of NGC 4151
Physical conditions in the narrow-line regions of M51 and NGC 4151
Probing the Ionization Structure of the Narrow-Line Region in the Seyfert 1 Galaxy NGC 4151
Resolved Mid-Infrared Emission in the Narrow-Line Region of NGC 4151
Simultaneous Ultraviolet and X-Ray Observations of the Seyfert Galaxy NGC 4151. II. Physical Conditions in the UV Absorbers
Space Telescope Imaging Spectrograph Echelle Observations of NGC 4151: Variable Ionization of the Intrinsic UV Absorbers
Space Telescope Imaging Spectrograph Echelle Observations of the Seyfert Galaxy NGC 4151: Physical Conditions in the Ultraviolet Absorbers
The Resolved Narrow-Line Region in NGC 4151
Instrument
STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1997-03-29T13:51:10Z/1997-05-25T01:44:45Z
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.