John H. Debes

In my 2009 paper on ISM sculpting of Debris Disks, I calculated some simple models that qualitatively fit three debris disks: HD 15115, HD 32297, and HD 61005. Contained here are fits files of surface brightness images of each of the models, assuming isotropic scattering of the dust grains. The headers contain information on the parameters used. The models were made using a simple N-body code that had a central star and massless test particles that served as proxies for dust particles, under the influence of a drag force proportional to v^2, the relative velocity of the grains and the perturbing ISM. The fits files have pixel sizes comparable to the NICMOS detector and have been convolved with a Tiny Tim PSF of the NIC-2 Camera PSF. Other configurations, such as for a ground-based observation can be made available upon request.

• Tar File of the HD 61005 models (Coming Soon!)
• Tar File of the HD 32297 models (Coming Soon!)
• Tar File of the HD 15115 models (Coming Soon!)