Modeling the Interstellar Medium-Stellar Wind Interactions of l Andromedae and e Indi
The Properties of the Local Interstellar Medium and the Interaction of the Stellar Winds of epsilon INDI and lambda Andromedae with the Interstellar Environment
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
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/1, HRS/2
Temporal Coverage
1994-08-31T13:43:28Z/1995-03-18T04:39:35Z
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, Alexander comma William R., 1996, 'UV SPECTROSCOPIC DETERMINATION OF THE D/H RATIO ALONG THE LINE OF SIGHT TOWARD EPSILON-IND AND LAMBDA-AND', 1.0, European Space Agency, https://doi.org/10.5270/esa-g4xydny