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Proper motions of USco T-type candidates

Citation

Lodieu, N and Ivanov, VD and Dobbie, PD, Proper motions of USco T-type candidates, Monthly Notices of the Royal Astronomical Society, 430, (3) pp. 1784-1789. ISSN 0035-8711 (2013) [Refereed Article]

Copyright Statement

Copyright 2013 The Authors

DOI: doi:10.1093/mnras/sts726

Abstract

We present new z - and H-band photometry and proper motion measurements for the five candidate very-low-mass T-type objects we recently proposed to be members of the nearest OB association with the Sun, Upper Scorpius (USco). These new data fail to corroborate our prior conclusions regarding their spectral types and affiliation with the USco population. We conclude that we may be in presence of a turnover in the mass function of USco taking place below 10-4MJup, depending on the age assigned to USco and the models used.

Item Details

Item Type:Refereed Article
Keywords:techniques: photometric – surveys – stars: luminosity function, mass function – infrared: stars
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Stellar Astronomy and Planetary Systems
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Dobbie, PD (Dr Paul Dobbie)
ID Code:84547
Year Published:2013
Web of Science® Times Cited:4
Deposited By:Mathematics and Physics
Deposited On:2013-05-17
Last Modified:2014-04-04
Downloads:0

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