The Observed Structure of Exosolar Kuiper Belts: Surprising Results and Unanswered Questions.

Details The Observed Structure of Exosolar Kuiper Belts: Surprising Results and Unanswered Questions. The Observed Structure of Exosolar Kuiper Belts: Surprising Results and Unanswered Questions.

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21110902k&link_type=abstract

American Astronomical Society, AAS Meeting #211, #109.02; Bulletin of the American Astronomical Society, Vol. 39, p.937

Astronomy and Astrophysics

Astronomy

Scientific paper

Dusty debris disks around nearby main sequence stars are the exosolar analogs of our Kuiper Belt. With recent advances in high-contrast imaging, 16 debris disks are now resolved at high-resolution in scattered light. A current snapshot of all resolved debris disks is available at www.disksite.com. I will review these new findings and examine the notion of separating debris disks into two categories: narrow belts and extended disks. However, these images also reveal a surprising diversity in debris disk structure. I will catalog the unusual or extreme properties of debris disks because they present new questions for future observations and theories to address.

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