SDSS J111010.01+011613.1: A New Planetary-mass T Dwarf Member of the AB Doradus Moving Group

Author(s)
Jonathan Gagne, Adam J. Burgasser, Jacqueline K. Faherty, David Lafreniere, Rene Doyon, Christine Nicholls
Abstract

We present a new radial velocity measurement that, together with a trigonometric parallax, proper motion and signs of low gravity from the literature, confirms that SDSS J111010.01+011613.1 is a new T5.5 bona fide member of AB Doradus. Fitting λ/Δλ ≈ 6000 Folded-port InfraRed Echellette spectroscopy in the 1.20-1.33 μm region to BT-Settl atmosphere models yielded a radial velocity of 7.5 ± 3.8 km s-1. At such a young age (110-130 Myr), current evolution models predict a mass of ~ 10-12 MJup, thus placing SDSS J1110+0116 well into the planetary-mass regime. We compare the fundamental properties of SDSS J1110+0116 with a sequence of seven recently identified M8-T5 brown dwarf bona fide or high-confidence candidate members of AB Doradus. We also note that its near-infrared J-K color is redder than field T5-T6 brown dwarfs, however its absolute J-band magnitude is similar to them. SDSS J1110+0116 is one of the few age-calibrated T dwarfs known to date, as well as one of the coolest bona fide members of a young moving group.

Organisation(s)
Department of Astrophysics
External organisation(s)
University of Montreal, University of California, San Diego, Carnegie Institution for Science, American Museum of Natural History
Journal
The Astrophysical journal Letters
Volume
808
No. of pages
6
ISSN
2041-8205
DOI
https://doi.org/10.1088/2041-8205/808/1/L20
Publication date
07-2015
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
ASJC Scopus subject areas
Astronomy and Astrophysics, Space and Planetary Science
Portal url
https://ucrisportal.univie.ac.at/en/publications/sdss-j111010010116131-a-new-planetarymass-t-dwarf-member-of-the-ab-doradus-moving-group(df69a59b-ca02-4a50-8d04-81460192da1e).html