Jerome Bouvier

TL;DR: The XMM-Newton Extended Survey of the Taurus Molecular Cloud (EST) presented in this article surveys the most populated =5 square degrees of TMC, using the XMMNewton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association.

TL;DR: The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) as discussed by the authors surveys the most populated 5 square degrees of Taurus star formation region, using the XMMNewton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association.

TL;DR: In this paper, the properties of pre-main-sequence objects in the Taurus molecular clouds as observed in 7 mid and far-infrared bands with the Spitzer Space Telescope were reported.

TL;DR: In this article, the authors investigate the accretion and outflow dynamics and their interaction from observations of the classical T T Tauri star AA Tau, and they find that most spectral and photometric diagnostics vary as expected from models of magnetically-channelled accretion in young stars, with a large scale magnetosphere tilted by 20 degrees onto the star spin axis.

TL;DR: In this article, a long time series of high-resolution HARPS spectra and simultaneous broad-band photometry was used to detect magnetospheric accretion and ejection processes in the nearly edge-on T Tauri star AA Tau.