Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-14
Science 310 (2005) 834
Astronomy and Astrophysics
Astrophysics
Published in Science 2005, vol 310, 834; 3 pages in final format, 4 figures + 8 pages Supporting Online Material. For final ty
Scientific paper
10.1126/science.1118042
The onset of planet formation in protoplanetary disks is marked by the growth and crystallization of sub-micron-sized dust grains accompanied by dust settling toward the disk mid-plane. Here we present infrared spectra of disks around brown dwarfs and brown dwarf candidates. We show that all three processes occur in such cool disks in a way similar or identical to that in disks around low- and intermediate-mass stars. These results indicate that the onset of planet formation extends to disks around brown dwarfs, suggesting that planet formation is a robust process occurring in most young circumstellar disks.
Apai Daniel
Bouwman Jeroen
Dullemond Cornelis Petrus
Henning Th
Natta Antonella
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