Interstellar Krypton Abundances: The Detection of Kiloparsec-scale Differences in Galactic Nucleosynthetic History
Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Singly Ionized Lead
Measurements of the f-Values of the Resonance Transitions of Ni II at 1317.217 and 1370.132 A
Oxygen Gas-Phase Abundance Revisited
Phosphorus in the diffuse interstellar medium
Rapid Temporal Variations of Interstellar Absorption Lines in the Carina Nebula
Space Telescope Imaging Spectrograph Observations of High-Velocity Interstellar Absorption-Line Profiles in the Carina Nebula
The abundance of boron in diffuse interstellar clouds
The Abundance of Boron in Diffuse Interstellar Clouds
The Abundance of Interstellar Boron
The Effective Temperatures of Hot Stars. II. The Early-O Types
The Variation of Magnesium Depletion with Line-of-Sight Conditions
Ultraviolet Survey of CO and H2 in Diffuse Molecular Clouds: The Reflection of Two Photochemistry Regimes in Abundance Relationships
Updated interstellar abundance studies and implications for dust models
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1998-03-19T21:44:55Z/1999-04-20T03:32:10Z
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, Danks et al., 2006, 'Studies of the Characteristics of the Interstellar Medium in the Carina Nebula', 1.0, European Space Agency, https://doi.org/10.5270/esa-bz3d7wu