Add to ORKGYoung, co-evolving stars, free of the obscuring effects of their formation region, exist near the Sun in loose associations with each constituent having a common motion through the Galaxy. These associations are collectively known as the nearby young moving groups (NYMGs). Most known members of the NYMGs are spectral type F, G, and K (1.5 - 0.7 MSun), with few of spectral type M (<0.7 MSun). Since low-mass M stars are the dominant stellar component of the universe (comprising ∼75% of all stars), the census of known members in the NYMGs is probably incomplete. The under-sampling of low-mass members is a consequence of their low-luminosity, wide sky distribution, and a lack of reliable youth indicators in the low-mass regime. NYMG members are...
Using the kinematically unbiased technique described in Binks, Jeffries & Maxted (2015), we present ...
<p>In this talk I present the latest results of a near-infrared spectroscopic follow-up of brown dwa...
Original article can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Socie...
Substellar members of young (lesssim150 Myr) moving groups are valuable benchmarks to empirically de...
We present Bayesian Analysis for Nearby Young AssociatioNs II (BANYAN II), a modified Bayesian anal-...
The last few decades have seen the discovery of many 10-100 Myr-old stars in moving groups within 10...
We present new radial velocity (RV) measurements for 11 candidate young very-low-mass stars and brow...
In the past decade many kinematic groups of young stars (<100 Myr) were discovered in the solar neig...
<p>We present Bayesian Analysis for Nearby Young AssociatioNs II (BANYAN II), a modified Bayesian an...
The census of young stars among nearby moving groups is far from complete, particularly at the low-m...
The latest results in the research of forming planetary systems have led several authors to compile ...
In order to compile a sample of ultracool dwarfs that will serve as benchmarks for testing theoretic...
Young stars in the solar neighborhood serve as nearby probes of stellar evolution and represent prom...
We present spectral and kinematic evidence that 2MASS J06085283−2753583 (M8.5γ) is a member of the β...
Optical spectroscopic observations are reported for 24 and 23, nearby, proper-motion-selected M-dwar...
Using the kinematically unbiased technique described in Binks, Jeffries & Maxted (2015), we present ...
<p>In this talk I present the latest results of a near-infrared spectroscopic follow-up of brown dwa...
Original article can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Socie...
Substellar members of young (lesssim150 Myr) moving groups are valuable benchmarks to empirically de...
We present Bayesian Analysis for Nearby Young AssociatioNs II (BANYAN II), a modified Bayesian anal-...
The last few decades have seen the discovery of many 10-100 Myr-old stars in moving groups within 10...
We present new radial velocity (RV) measurements for 11 candidate young very-low-mass stars and brow...
In the past decade many kinematic groups of young stars (<100 Myr) were discovered in the solar neig...
<p>We present Bayesian Analysis for Nearby Young AssociatioNs II (BANYAN II), a modified Bayesian an...
The census of young stars among nearby moving groups is far from complete, particularly at the low-m...
The latest results in the research of forming planetary systems have led several authors to compile ...
In order to compile a sample of ultracool dwarfs that will serve as benchmarks for testing theoretic...
Young stars in the solar neighborhood serve as nearby probes of stellar evolution and represent prom...
We present spectral and kinematic evidence that 2MASS J06085283−2753583 (M8.5γ) is a member of the β...
Optical spectroscopic observations are reported for 24 and 23, nearby, proper-motion-selected M-dwar...
Using the kinematically unbiased technique described in Binks, Jeffries & Maxted (2015), we present ...
<p>In this talk I present the latest results of a near-infrared spectroscopic follow-up of brown dwa...
Original article can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Socie...