A Model of the C IV l l1548, 1550 Doublet Line in T Tauri Stars
PENELLOPE. II. CVSO 104: A pre-main sequence close binary with an optical companion in Ori OB1
PENELLOPE: The ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES). I. Survey presentation and accretion properties of Orion OB1 and s-Orionis
PENELLOPE: VIII. Veiling and extinction variations of V505 Ori
PENELLOPE: VII. Revisiting empirical relations to measure accretion luminosity
PENELLOPE. V. The magnetospheric structure and the accretion variability of the classical T Tauri star HM Lup
The ODYSSEUS Survey. Characterizing Magnetospheric Geometries and Hotspot Structures in T Tauri Stars
The ODYSSEUS Survey. Spatial Correlation of Magnetospheric Inclinations Points to Parsec-scale Star-Cloud Connection
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-type T Tauri stars in Orion OBIb Star Forming Region', 1.0, European Space Agency, https://doi.org/10.57780/esa-wutzcnx