A Reanalysis of the SWP-HI IUE Observations of Capella
Deceleration of Interstellar Hydrogen at the Heliospheric Interface
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
Dissecting Capellas Corona: GHRS Spectra of the Fe XXI l1354 and He II l1640 Lines from Each of the Capella Stars
Goddard High-Resolution Spectrograph Observations of the Local Interstellar Medium and the Deuterium/Hydrogen Ratio along the Line of Sight toward Capella
Local Clouds : Distribution, Density and Kinematics Through Ground-Based and HST Spectroscopy
Local Cloud structure from HST-GHRS
Measurements of the interstellar gas
The Transition Regions of Capella
Two New Low Galactic D/H Measurements from the Far Ultraviolet Spectroscopic Explorer
Ultraviolet observations of stellar coronae : early results from HST.
What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument
HRS, HRS/1, HRS/2
Temporal Coverage
1991-04-15T05:11:37Z/1991-04-15T13:49:14Z
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 comma Jeffrey L., 1992, 'LOCAL INTERSTELLAR MEDIUM AND D/H RATIO -- CYCLE 0', 1.0, European Space Agency, https://doi.org/10.5270/esa-tj06osp