Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud
Optically thick structure in early B-type supergiant stellar winds at low metallicities
Physical conditions in the diffuse interstellar medium of local and high-redshift galaxies: measurements based on the excitation of H2 rotational and C I fine-structure levels
Probing the Dust Responsible for Small Magellanic Cloud Extinction
StarCAT: A Catalog of Space Telescope Imaging Spectrograph Ultraviolet Echelle Spectra of Stars
Thermal Pressures in the Interstellar Medium of the Magellanic Clouds
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2002-09-22T05:04:01Z/2003-10-17T03:33:47Z
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, Gordon comma Karl D., 2006, 'Probing the Grains Responsible for Extinction Using Small Magellanic Cloud Sightlines', 1.0, European Space Agency, https://doi.org/10.5270/esa-mkgt7j3