Abundances and Depletions of Neutron-capture Elements in the Interstellar Medium
A Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium
Extreme resonance line profile variations in the ultraviolet spectra of NGC 1624-2: probing the giant magnetosphere of the most strongly magnetized known O-type star
Hubble Space Telescope Survey of Interstellar 12CO/13CO in the Solar Neighborhood
Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Singly Ionized Lead
The abundance of boron in diffuse interstellar clouds
The Abundance of Boron in Diffuse Interstellar Clouds
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2001-09-16T19:55:54Z/2001-09-16T21:14:57Z
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, Boggess comma Albert, 2006, 'Probing the Physical Conditoins of an Interstellar Bubble around an O Star', 1.0, European Space Agency, https://doi.org/10.5270/esa-4jmp3rb