Chandra, EUVE, HST, and VLA Multiwavelength Campaign on HR 1099: Instrumental Capabilities, Data Reduction, and Initial Results
Elemental Abundances and Ionization States within the Local Interstellar Cloud Derived from Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer Observations of the Capella Line of Sight
Space Telescope Imaging Spectrograph Survey of Far-Ultraviolet Coronal Forbidden Lines in Late-Type Stars
The Capella Giants and Coronal Evolution across the Hertzsprung Gap
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
UV and EUV observations of stellar coronal structure and activity
What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1999-09-12T18:07:40Z/1999-09-12T23:00:21Z
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, Drake comma Jeremy J., 1999, 'The First Comprehensive High Spectral Resolution Study of Stellar Coronae: The 1999 Chandra, HST, EUVE, SAX and VLA Capella Campaign', 1.0, European Space Agency, https://doi.org/10.5270/esa-kivwrt9