The identification and characterisation of low-mass binaries is of importance for a range of astrophysical investigations. Low-mass binaries in young (∼10–100 Myr) moving groups (YMGs) in the solar neighborhood are of particular significance as they provide unique opportunities to calibrate stellar models and evaluate the ages and coevality of the groups themselves. Low-mass M-dwarfs have pre-main sequence life times on the order of ∼100 Myr and therefore are continually evolving along a mass-luminosity track throughout the YMG phase, providing ideal laboratories for precise isochronal dating, if a model-independent dynamical mass can be measured. AstraLux lucky imaging multiplicity surveys have recently identified hundreds of new YMG low-m...
We present the identification of two previously known young objects in the solar neighbourhood as a...
We present spectral and kinematic evidence that 2MASS J06085283–2753583 (M8.5γ) is a member of the β...
Low-mass stars exhibit substantial pre-main sequence evolution during the first ∼100 Myr of their li...
The identification and characterisation of low-mass binaries is of importance for a range of astroph...
The solar galactic neighborhood contains a number of young co-moving associations of stars (known as...
We present new radial velocity (RV) measurements for 11 candidate young very-low-mass stars and brow...
Copyright © 2015. The American Astronomical Society. All rights reserved.We present optical and near...
We present optical and near-infrared adaptive optics (AO) imaging and spectroscopy of 13 ultracool (...
We present optical and near-infrared adaptive optics (AO) imaging and spectroscopy of 13 ultracool (...
We present optical and near-infrared adaptive optics (AO) imaging and spectroscopy of 13 ultracool (...
Low-mass stars exhibit substantial pre-main sequence evolution during the first ̃100 Myr of their li...
The solar galactic neighborhood contains a number of young co-moving associations of stars (known as...
Young M-type binaries are particularly useful for precise isochronal dating by taking advantage of t...
We present the results of a radial velocity (RV) survey of 14 brown dwarfs (BDs) and very low-mass ...
Young M-type binaries are particularly useful for precise isochronal dating by taking advantage of t...
We present the identification of two previously known young objects in the solar neighbourhood as a...
We present spectral and kinematic evidence that 2MASS J06085283–2753583 (M8.5γ) is a member of the β...
Low-mass stars exhibit substantial pre-main sequence evolution during the first ∼100 Myr of their li...
The identification and characterisation of low-mass binaries is of importance for a range of astroph...
The solar galactic neighborhood contains a number of young co-moving associations of stars (known as...
We present new radial velocity (RV) measurements for 11 candidate young very-low-mass stars and brow...
Copyright © 2015. The American Astronomical Society. All rights reserved.We present optical and near...
We present optical and near-infrared adaptive optics (AO) imaging and spectroscopy of 13 ultracool (...
We present optical and near-infrared adaptive optics (AO) imaging and spectroscopy of 13 ultracool (...
We present optical and near-infrared adaptive optics (AO) imaging and spectroscopy of 13 ultracool (...
Low-mass stars exhibit substantial pre-main sequence evolution during the first ̃100 Myr of their li...
The solar galactic neighborhood contains a number of young co-moving associations of stars (known as...
Young M-type binaries are particularly useful for precise isochronal dating by taking advantage of t...
We present the results of a radial velocity (RV) survey of 14 brown dwarfs (BDs) and very low-mass ...
Young M-type binaries are particularly useful for precise isochronal dating by taking advantage of t...
We present the identification of two previously known young objects in the solar neighbourhood as a...
We present spectral and kinematic evidence that 2MASS J06085283–2753583 (M8.5γ) is a member of the β...
Low-mass stars exhibit substantial pre-main sequence evolution during the first ∼100 Myr of their li...