Deuterium Abundance in the Local ISM and Possible Spatial Variations
HST-GHRS observations of a Piscis Austrini. Evidence of no gas content in the circumstellar environment.
Local Clouds : Distribution, Density and Kinematics Through Ground-Based and HST Spectroscopy
Local Cloud structure from HST-GHRS
Physical structure of the local interstellar medium
The interstellar cloud surrounding the Sun: a new perspective
The Structure of the Local Interstellar Medium. I. High-Resolution Observations of Fe II, Mg II, and Ca II toward Stars within 100 Parsecs
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
The three-dimensional physical structure of the local interstellar medium
Instrument
HRS, HRS/2
Temporal Coverage
1993-01-23T11:48:48Z/1993-11-03T16:57:47Z
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, Ferlet et al., 1994, 'PHYSICAL CONDITIONS OF INTERSTELLAR GAS WITHIN 50 PARSECS', 1.0, European Space Agency, https://doi.org/10.5270/esa-yhex0te