Analysis of Helium-rich White Dwarfs Polluted by Heavy Elements in the Gaia Era
Atomic Physics with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. V. Oscillator Strengths for Neutral Carbon Lines below 1200 A
Nonthermal Chemistry in Diffuse Clouds with Low Molecular Abundances
The Abundance of Interstellar Krypton
The Homogeneity of Interstellar Krypton in the Galactic Disk
Wide Field Planetary Camera 2 Photometry of the Bright, Mysterious White Dwarf Procyon B
Instrument
HRS, HRS/2
Temporal Coverage
1994-04-17T02:56:41Z/1995-03-21T03:24:55Z
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, Cardelli comma Jason A., 1996, 'THE INTERSTELLAR ABUNDANCE OF KRYPTON: CYCLE 4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-1aglhmc