2022 (v1)
Journal article
The disk of FU Orionis viewed with MATISSE/VLTI. First interferometric observations in L and M bands
Aims: We studied the accretion disk of the archetypal eruptive young star FU Orionis with the use of mid-infrared interferometry, which enabled us to resolve the innermost regions of the disk down to a spatial resolution of 3 milliarcseconds (mas) in the L band, that is, within 1 au of the protostar. Methods: We used the interferometric...
Uploaded on: December 3, 2022