Mathematics – Logic
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008dps....40.1106f&link_type=abstract
American Astronomical Society, DPS meeting #40, #11.06; Bulletin of the American Astronomical Society, Vol. 40, p.402
Mathematics
Logic
Scientific paper
We have taken existing dust morphology modeling software, ZODIPIC (Kuchner et al. 2007) and modified the opacity data to reflect the species detected in comets from the Deep Impact mission, the Spitzer survey of comets, STARDUST, and bright exo-planetary dust spectra. Opacities from multiple chemical species were adapted to the ZODIPIC code and now contain spectra that can match the existing spectra from the debris disk systems. User supplied coefficients can now modify pre-programmed spectral species to match morphological outputs with desired empirical expectations. This tool can aid in generating expectations for direct or indirect observations of exoplanetary debris disks. We show example morphological models of silicate rich (e.g., HD69830, Beichman et al. 2005) and carbon-rich (Beta Pic like, Roberge et al. 2007) systems.
Fraine Jonathan
Kuchner Marc
Lisse Carey Michael
Stark Christopher C.
No associations
LandOfFree
Numerical Modeling of Dusty Disk System Morphologies With Deep Impact Derived Opacities does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Numerical Modeling of Dusty Disk System Morphologies With Deep Impact Derived Opacities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical Modeling of Dusty Disk System Morphologies With Deep Impact Derived Opacities will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1436549