Deuterium Abundance in the Local ISM and Possible Spatial Variations
GHRS observations of Sirius-A I. Interstellar clouds toward Sirius and Local Cloud ionization
Heliospheric and it astrospheric hydrogen absorption towards Sirius: no need for interstellar hot gas
HST-GHRS observations of Sirius A. III. Detection of a stellar wind from Sirius A
Local Clouds : Distribution, Density and Kinematics Through Ground-Based and HST Spectroscopy
Local Cloud structure from HST-GHRS
Possible detection of a diffuse interstellar cloud boundary. II. HST-GHRS observations of Sirius A.
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
The Three-dimensional Structure of the Warm Local Interstellar Medium. II. The Colorado Model of the Local Interstellar Cloud
The Three-dimensional Structure of the Warm Local Interstellar Medium. I. Methodology
UV Spectral Synthesis of Vega
Instrument
HRS, HRS/2
Temporal Coverage
1992-08-10T13:09:36Z/1992-08-15T23:22:10Z
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, Lallement comma Rosine, 1993, 'INTERPLANETARY/INTERSTELLAR GAS CONNECTION: SEARCH FOR THE LOCAL CLOUD', 1.0, European Space Agency, https://doi.org/10.5270/esa-vjg4f8s