Balmer and He I Absorption in the Nuclear Spectrum of NGC 4151
Characterizing Transition Temperature Gas in the Galactic Corona
C II Radiative Cooling of the Diffuse Gas in the Milky Way
Feedback from Mass Outflows in Nearby Active Galactic Nuclei. II. Outflows in the Narrow-line Region of NGC 4151
Investigating the Narrow-line Region Dynamics in Nearby Active Galaxies
Kinematics of the narrow-line regions in the Seyfert galaxies NGC 4151 and NGC 1068
Mapping the Kinematics of the Narrow-Line Region in the Seyfert Galaxy NGC 4151
Mass Outflow from the Nucleus of the Seyfert 1 Galaxy NGC 4151
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Radial Velocity Offsets Due to Mass Outflows and Extinction in Active Galactic Nuclei
Simultaneous Ultraviolet and X-Ray Observations of the Seyfert Galaxy NGC 4151. II. Physical Conditions in the UV Absorbers
Spatially Resolved Narrow-Line Region Kinematics in Active Galactic Nuclei
The Milky Way halo as a QSO absorption-line system. New results from an HST/STIS absorption-line catalogue of Galactic high-velocity clouds
The non-constant slope of the C IV Baldwin effect in NGC 4151
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-06-15T10:23:04Z/2001-04-14T03:59:32Z
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, Hutchings comma John, 2006, 'STIS Key Project: The nuclear region of NGC 4151 Observations', 1.0, European Space Agency, https://doi.org/10.5270/esa-ep30g0p