Deuterium Abundance in the Local ISM and Possible Spatial Variations
Deuterium and the Local Interstellar Medium Properties for the Procyon and Capella Lines of Sight
Deuterium Observations in the Galaxy
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Local Clouds : Distribution, Density and Kinematics Through Ground-Based and HST Spectroscopy
Local Cloud structure from HST-GHRS
Mg II h + k Flux--Rotational Period Correlation for G-type Stars
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 three-dimensional physical structure of the local interstellar medium
Two New Low Galactic D/H Measurements from the Far Ultraviolet Spectroscopic Explorer
What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument
HRS, HRS/2
Temporal Coverage
1993-04-29T00:55:53Z/1993-09-19T13:02:05Z
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, Linsky et al., 1994, 'LOCAL INTERSTELLAR MEDIUM AND D/H RATIO -- CYCLE 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-gv7zr9t