Meridional flows in the disk around a young star.


Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
10 2019
Historique:
received: 22 03 2019
accepted: 25 07 2019
entrez: 18 10 2019
pubmed: 18 10 2019
medline: 18 10 2019
Statut: ppublish

Résumé

Protoplanetary disks are known to possess a variety of substructures in the distribution of their millimetre-sized grains, predominantly seen as rings and gaps

Identifiants

pubmed: 31619790
doi: 10.1038/s41586-019-1642-0
pii: 10.1038/s41586-019-1642-0
doi:

Types de publication

Journal Article Research Support, U.S. Gov't, Non-P.H.S. Research Support, Non-U.S. Gov't

Langues

eng

Sous-ensembles de citation

IM

Pagination

378-381

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Auteurs

Richard Teague (R)

Department of Astronomy, University of Michigan, Ann Arbor, MI, USA. rteague@umich.edu.

Jaehan Bae (J)

Department of Terrestrial Magnetism, Carnegie Institution for Science, Washington, DC, USA.

Edwin A Bergin (EA)

Department of Astronomy, University of Michigan, Ann Arbor, MI, USA.

Classifications MeSH