Completing the MIPS GTO Debris Disk Sample

Details Completing the MIPS GTO Debris Disk Sample Completing the MIPS GTO Debris Disk Sample

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop30566r&link_type=abstract

Spitzer Proposal ID #30566

Physics

Scientific paper

We will measure 15 stars at 70 micron to add to our understanding of debris disk evolution. These stars either have poor Spitzer measurements due to instrumental problems, or have measurements with ISO that need to be confirmed. Most of them are late B or early A stars, and will add to the statistical robustness of our program concentrating on the evolution of disks around such stars with age.

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