Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
Lya Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems
Measurement of interstellar extinction for classical T Tauri stars using far-UV H2 line fluxes
Optically thick structure in early B-type supergiant stellar winds at low metallicities
The Gaseous Blowout of the 30 Doradus Starburst Region in the LMC
The Radial Distribution and Excitation of H2 around Young Stars in the HST-ULLYSES Survey
Thermal Pressures in the Interstellar Medium away from Stellar Environments
The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Directors Discretionary Program with Hubble. I. Goals, Design, and Initial Results
X-Shooting ULLYSES: Massive stars at low metallicity. II. DR1: Advanced optical data products for the Magellanic Clouds
X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars
X-Shooting ULLYSES: Massive stars at low metallicity: VII. Stellar and wind properties of B supergiants in the Small Magellanic Cloud
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2020-09-05T18:51:13Z/2020-09-30T11:13:41Z
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.
