Warm Dust Around Main-Sequence Stars Discovered with 2MASS

Details Warm Dust Around Main-Sequence Stars Discovered with 2MASS Warm Dust Around Main-Sequence Stars Discovered with 2MASS

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..324..259f&link_type=abstract

Debris Disks and the Formation of Planets: A Symposium in Memory of Fred Gillett, ASP Conference Series, Vol. 324, Proceedings o

Astronomy and Astrophysics

Astronomy

Scientific paper

We report results of ground-based 10 μm photometry of main-sequence stars with warm (Tdust ˜ 300 K) circumstellar dust. We originally discovered these dust systems through IRAS 12 μm excess emission relative to 2MASS J, H, and Ks photospheric emission. We possibly confirmed circumstellar 10 μm excess emission from four sources.

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