The Onset of Planet Formation in Brown Dwarf Disks

dc.creatorApai, D.
dc.creatorPascucci, I.
dc.creatorBouwman, J.
dc.creatorNatta, A.
dc.creatorHenning, Th.
dc.creatorDullemond, C. P.
dc.date2005-11-14
dc.date.accessioned2026-07-07T06:45:06Z
dc.date.available2026-07-07T06:45:06Z
dc.descriptionThe 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.
dc.descriptionPublished in Science 2005, vol 310, 834; 3 pages in final format, 4 figures + 8 pages Supporting Online Material. For final typeset, see http://www.sciencemag.org/cgi/content/abstract/310/5749/834?etoc
dc.identifierhttps://arxiv.org/abs/astro-ph/0511420
dc.identifierhttp://arxiv.org/abs/astro-ph/0511420
dc.identifierScience 310 (2005) 834
dc.identifierdoi:10.1126/science.1118042
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102962
dc.subjectAstrophysics
dc.titleThe Onset of Planet Formation in Brown Dwarf Disks
dc.typetext

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