Ph.D., Vanderbilt University, 2010
Alicia Aarnio aims, with her research, to understand the innermost regions of disks around young, intermediate mass stars: inner disk structure; geometry; and how material is moving within and out of the star-disk system.
Mass Loss in Pre-Main Sequence Stars via Coronal Mass Ejections and Implications for Angular Momentum Loss, Aarnio, Matt, and Stassun; ApJ, 2012
Mechanical Equilibrium of Hot, Large-Scale Magnetic Loops on T Tauri Stars, Aarnio, Llama, Jardine, and Gregory; MNRAS, 2012
Solar Flares and Coronal Mass Ejections: A Statistically Determined Flare Flux-CME Mass Correlation, Aarnio, Stassun, Hughes, and McGregor; Solar Physics, 2011
A Search for Star-Disk Interaction among the Strongest X-ray Flaring Stars in the Orion Nebula Cluster, Aarnio, Stassun, and Matt; ApJ, 2010
T Tauri Angular Momentum Loss via Large Scale Eruptive Flaring Events, Aarnio, Stassun, and Matt; AIPC, 2009