2 papers
astro-ph.SR2025
The mass distribution of clumpy accretion onto the nearby young star TW Hya
Tao Ji, Javier Serna, Gregory J. Herczeg +12
The proliferation of high time-resolution and decades-long monitoring of classical T Tauri stars provides a vast opportunity to test the variability of the star-disk connections. H…
astro-ph.SR2025
Spinning-down RU Lup. Constraints on the physics of the outflow from high-resolution spectroscopy
A. Armeni, B. Stelzer, A. Frasca +4
Magnetic winds are a key mechanism for angular momentum removal in young stars. In this work, we aim at characterizing the multi-component outflow of RU Lup. The unprecedented high…