The onset of planet formation in brown dwarf disks

Daniel Apai, Ilaria Pascucci, Jeroen Bouwman, Antonella Natta, Thomas Henning, Cornelis P. Dullemond

143 Scopus citations

Abstract

The onset of planet formation in protoplanetary disks is marked by the growth and crystallization of sub-micrometer-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.

Original languageEnglish (US)
Pages (from-to)834-836
Number of pages3
JournalScience
Volume310
Issue number5749
DOIs
Publication statusPublished - Nov 4 2005

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Cite this

The onset of planet formation in brown dwarf disks. / Apai, Daniel; Pascucci, Ilaria; Bouwman, Jeroen; Natta, Antonella; Henning, Thomas; Dullemond, Cornelis P.

In: Science, Vol. 310, No. 5749, 04.11.2005, p. 834-836.

Research output: Contribution to journalArticle