SCExAO/CHARIS Multi-Wavelength, High-Contrast Imaging of the BD+45598 Debris Disk
arXiv:2405.04521 · doi:10.3847/1538-3881/ad4864
Abstract
We present a multi-wavelength (1.16m-2.37m) view of the debris disk around BD+45598, using the Subaru Coronagraphic Extreme Adaptive Optics system paired with the Coronagraphic High Angular Resolution Imaging Spectrograph. With an assumed age of 23 Myr, this source allows us to study the early evolution of debris disks and search for forming planets. We fit a scattered light model to our disk using a differential evolution algorithm, and constrain its geometry. We find the disk to have a peak density radius of au, an inclination of , and position angle . While we do not detect a substellar companion in the disk, our calculated contrast limits indicate sensitivity to planets as small as at a projected separation of 12 au of the star, and as small as beyond 38 au. When measuring intensity as a function of wavelength, the disk color constrains the minimum dust grain size within a range of to 1.01m.
arXiv comment22 pages, 12 figures; Accepted to AJ
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