Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
HST/COS Spectra of the Wind Lines of VFTS 102 and 285
METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. II. Variations of Interstellar Depletions and Dust-to-gas Ratio within the LMC
Optically thick structure in early B-type supergiant stellar winds at low metallicities
Optical spectroscopy of the blue supergiant Sk-69deg 279 and its circumstellar shell with SALT
The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses
The impact of satellite trails on Hubble Space Telescope observations
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, Roman-Duval comma Julia Christine, 2013, 'A Direct CO/H2 Abundance Measurement in Diffuse and Translucent LMC and SMC Molecular Clouds', 1.0, European Space Agency, https://doi.org/10.5270/esa-1bksbe0