A Model of the C IV l l1548, 1550 Doublet Line in T Tauri Stars
An Ultraviolet Study of CO Chemistry in the Magellanic Clouds
Evidence of a Disk Wind Origin for Fluorescent H2 in Classical T Tauri Stars
PENELLOPE. IV. A comparison between optical forbidden lines and H2 UV lines in the Orion OB1b and s-Ori associations
PENELLOPE: VII. Revisiting empirical relations to measure accretion luminosity
The ODYSSEUS Survey. Characterizing Magnetospheric Geometries and Hotspot Structures in T Tauri Stars
The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109
The ODYSSEUS Survey. Spatial Correlation of Magnetospheric Inclinations Points to Parsec-scale Star-Cloud Connection
The ODYSSEUS Survey. Using Accretion and Stellar Rotation to Reveal the Star-Disk Connection in T Tauri Stars
The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Directors Discretionary Program with Hubble. I. Goals, Design, and Initial Results
The wind properties of O-type stars at sub-SMC metallicity
Towards a Comprehensive View of Accretion, Inner Disks, and Extinction in Classical T Tauri Stars: An ODYSSEUS Study of the Orion OB1b Association
Using the Ca II Lines in T Tauri Stars to Infer the Abundance of Refractory Elements in the Innermost Disk Region
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, 2020, 'ULLYSES K and M-type T Tauri stars in Orion OBIb Star Forming Region', 1.0, European Space Agency, https://doi.org/10.57780/esa-kbp0ceu