A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
Optically thick structure in early B-type supergiant stellar winds at low metallicities
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. I. Project description
X-Shooting ULLYSES: Massive Stars at low metallicity: IX. Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud
X-Shooting ULLYSES: Massive stars at low metallicity: V. Effect of metallicity on surface abundances of O stars
X-Shooting ULLYSES: Massive stars at low metallicity: VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
X-Shooting ULLYSES: Massive stars at low metallicity: XIII. Testing the bi-stability jump in the Large Magellanic Cloud
Instrument
STIS, STIS/CCD
Temporal Coverage
2020-10-07T02:20:49Z/2022-09-13T00:38:17Z
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, Massa, 2022, 'An NUV SNAP program to supplement and enhance the value of the ULLYSES OB star legacy data.', 1.0, European Space Agency, https://doi.org/10.5270/esa-2nmyrd6