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20072009
most citedExploring the substellar temperature regime down to ~550K

124 citations · 723 across the 12 of their papers we have counts for

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15 papers · 1 filter

astro-ph200884 cited

First Confirmed Detection of a Bipolar Molecular Outflow from a Young Brown Dwarf

Ngoc Phan-Bao, Basmah Riaz, Chin-Fei Lee +6

Studying the earliest stages in the birth of stars is crucial for understanding how they form. Brown dwarfs with masses between that of stars and planets are not massive enough to…

astro-ph200842 cited

A deep look into the cores of young clusters I. sigma-Orionis

H. Bouy, N. Huelamo, E. L. Martin +9

Nearby young clusters are privileged places to study the star formation history. Over the last decade, the sigma-Orionis cluster has been a prime location for the study of young ve…

astro-ph2008124 cited

Exploring the substellar temperature regime down to ~550K

Ben Burningham, D. J. Pinfield, S. K. Leggett +15

We report the discovery of three very late T dwarfs in the UKIRT Infrared Deep Sky Survey (UKIDSS) Third Data Release: ULAS J101721.40+011817.9 (ULAS1017), ULAS J123828.51+095351.3…

astro-ph200850 cited

IPHAS discoveries of young stars towards Cyg OB2 and its southern periphery

Jorick S. Vink, Janet E. Drew, Danny Steeghs +5

We report on the discovery of over 50 strong Halpha emitting objects towards the large OB association Cyg OB2 and the HII region DR 15 on its southern periphery. This was achieved…

astro-ph200824 cited

Follow-up observations of binary ultra-cool dwarfs

H. Bouy, E. L. Martin, W. Brandner +12

Astrometric observations of resolved binaries provide estimates of orbital periods and will eventually lead to measurement of dynamical masses. Only a few very low mass star and br…

astro-ph2007105 cited

Discovery of a wide companion near the deuterium burning mass limit in the Upper Scorpius association

V. J. S. Bejar, M. R. Zapatero Osorio, A. Perez-Garrido +5

We present the discovery of a companion near the deuterium burning mass limit located at a very wide distance, at an angular separation of 4.6+/-0.1 arcsec (projected distance of ~…