First millimeter detection of the disk around a young, isolated, planetary-mass object

OTS44 is one of only four free-floating planets known to have a disk. We have previously shown that it is the coolest and least massive known free-floating planet (\(\sim\)12 M\(_{\rm Jup}\)) with a substantial disk that is actively accreting. We have obtained Band 6 (233 GHz) ALMA continuum data of...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2017-05
Hauptverfasser:	Bayo, Amelia, Joergens, Viki, Liu, Yao, Brauer, Robert, Olofsson, Johan, Arancibia, Javier, Pinilla, Paola, Wolf, Sebastian, Ruge, Jan Philipp, Henning, Thomas, Natta, Antonella, Johnston, Katharine G, Bonnefoy, Mickael, Beuther, Henrik, Chauvin, Gael
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Brown dwarf stars Brown dwarfs Dust Physics - Astrophysics of Galaxies Physics - Earth and Planetary Astrophysics Physics - Solar and Stellar Astrophysics Planet detection Rogue planets Uniqueness
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!