The onset of planet formation in brown dwarf disks

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

Research output: Contribution to journalArticle

146 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
StatePublished - Nov 4 2005

ASJC Scopus subject areas

  • General

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    Apai, D., Pascucci, I., Bouwman, J., Natta, A., Henning, T., & Dullemond, C. P. (2005). The onset of planet formation in brown dwarf disks. Science, 310(5749), 834-836. https://doi.org/10.1126/science.1118042