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Related papers: A search for southern ultracool dwarfs in young mo…

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Recent massive sky surveys in different bandwidths are providing new opportunities to modern astronomy. The Virtual Observatory (VO) represents the adequate framework to handle the huge amount of information available and filter out data…

Solar and Stellar Astrophysics · Physics 2016-03-01 Esther Pérez-Fernández , Ana Ulla , Enrique Solano , Raquel Oreiro , Carlos Rodrigo

Ultracool dwarfs consist of lowest-mass stars and brown dwarfs. Their interior is fully convective, different from that of the partly-convective Sun-like stars. Magnetic field generation process beneath the surface of ultracool dwarfs is…

Solar and Stellar Astrophysics · Physics 2025-12-10 Yue Xiang , Shenghong Gu , Dongtao Cao

We present results from our continuing program to identify new, low-mass, members of the nearby young moving groups (NYMGs) using a proper motion selection algorithm and various observational techniques. We have three goals: 1) To provide…

Solar and Stellar Astrophysics · Physics 2015-05-18 Joshua E. Schlieder , Sébastien Lépine , Michal Simon

The Gaia data release 2 (DR2) contains $>$6000 objects with parallaxes $(Plx+3\times{e\_Plx})>50$mas placing them within 20pc from the Sun. Since the expected numbers extrapolating the well-known 10pc census are much lower, nearby Gaia…

Solar and Stellar Astrophysics · Physics 2020-05-13 Ralf-Dieter Scholz

We present a new method to derive the age of young (<0.7 Gyr) L dwarfs based on their near-infrared photometry, colours, and distances. The method is based on samples of L dwarfs belonging to the Upper Sco association (5 Myr), the Alpha Per…

Astrophysics · Physics 2009-11-13 R. F. Jameson , N. Lodieu , S. L. Casewell , N. P. Bannister , P. D. Dobbie

Rotationally modulated photometric variability of ultracool dwarfs encodes key information about cloud structure and temperature contrasts. Large homogeneous optical datasets are crucial for linking atmospheric heterogeneity to fundamental…

Solar and Stellar Astrophysics · Physics 2026-05-05 Haomiao Huang , Shu Wang , Xiaodian Chen , Zhijun Tu , Jifeng Liu

We observe 14 young low-mass substellar objects in young moving groups using the SINFONI IFS with LGS-AO to detect and characterize 3 candidate binary systems. Together with the adopted young moving group ages we employ isochrones from…

Solar and Stellar Astrophysics · Physics 2019-07-24 Per Calissendorff , Markus Janson , Rubén Asensio-Torres , Rainer Köhler

We present the results of a deep-imaging search for wide companions to low-mass stars and brown dwarfs using NSFCam on IRTF. We searched a sample of 132 M7-L8 dwarfs to magnitude limits of $J \sim 20.5$ and $K \sim 18.5$, corresponding to…

We present a wide-field photometric survey covering ~200 deg^2 toward the Upper Scorpius OB association. Data taken in the R and I bands with the Quest-2 camera on the Palomar 48-inch telescope were combined with the 2MASS JHK survey and…

Astrophysics · Physics 2009-11-11 Catherine Slesnick , John Carpenter , Lynne Hillenbrand

We identify 806 ultra-cool dwarfs from their SDSS riz photometry (of which 34 are newly discovered L dwarfs) and obtain proper motions through cross matching with UKIDSS and 2MASS. Proper motion and distance constraints show that nine of…

We have estimated the age of the young moving group TW Hydrae Association, a cohort of a few dozen stars and brown dwarfs located near the Sun which share the same kinematic properties and, presumably, the same origin and age. The…

Astrophysics · Physics 2016-07-01 David Barrado y Navascues

Studies of cool white dwarfs in the solar neighbourhood have placed a limit on the age of the Galactic disk of 8-9 billion years. However, determining their cooling ages requires the knowledge of their effective temperatures, masses, radii,…

Here we present 1584 new southern proper motion systems with mu > 0.18 "/yr and 16.5 > R_59F > 18.0. This search complements the six previous SuperCOSMOS-RECONS (SCR) proper motion searches of the southern sky for stars within the same…

Solar and Stellar Astrophysics · Physics 2015-05-28 Mark R. Boyd , Todd J. Henry , Wei-Chun Jao , John P. Subasavage , Nigel C. Hambly

We report on initial results from a Spitzer program to search for very low-mass brown dwarfs in Ophiuchus. This program is an extension of an earlier study by Allers et al. which had resulted in an extraordinary success rate, 18 confirmed…

Solar and Stellar Astrophysics · Physics 2015-05-19 Paul M. Harvey , Daniel T. Jaffe , Katelyn Allers , Michael Liu

(abridged) We present high-resolution echelle spectroscopy of a photometricaly-selected sample if thirty-nine dwarfs with spectral types between M6.5 and L0.5. Two stars, 2MASSI 0253202+271333 and 2MASSW 0952219-192431, are double-lined…

Astrophysics · Physics 2010-04-29 I. Neill Reid , J. Davy Kirkpatrick , J. Liebert , J. E. Gizis , C. C. Dahn , D. G. Monet

We identify and investigate known ultracool stars and brown dwarfs that are being observed or indirectly constrained by the Gaia mission. These objects will be the core of the Gaia ultracool dwarf sample composed of all dwarfs later than M7…

Solar and Stellar Astrophysics · Physics 2017-05-31 R. L. Smart , F. Marocco , J. A. Caballero , H. R. A. Jones , D. Barrado , J. C. Beamin , D. J. Pinfield , L. M. Sarro

Little is known about the existence of extrasolar planets around ultracool dwarfs. Furthermore, binary stars with Sun-like primaries and very low-mass binaries composed of ultracool dwarfs show differences in the distributions of mass ratio…

Solar and Stellar Astrophysics · Physics 2015-06-16 J. Sahlmann , P. F. Lazorenko , D. Segransan , E. L. Martin , D. Queloz , M. Mayor , S. Udry

We present the results of a 9.3 square degree infrared (ZYJHK) survey in the Upper Scorpius association extracted from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Cluster Survey Early Data Release. We have selected a total of 112…

Astrophysics · Physics 2009-11-11 N. Lodieu , N. C. Hambly , R. F. Jameson

We present results from the PARallaxes of Southern Extremely Cool objects (PARSEC) program, an observational program begun in April 2007 to determine parallaxes for 122 L and 28 T southern hemisphere dwarfs using the Wide Field Imager on…

We present a kinematic analysis of 152 low surface gravity M7-L8 dwarfs by adding 8 parallaxes, 38 radial velocities, and 19 proper motions. We find 39 objects to be high-likelihood or bona fide members of nearby moving groups, 92 objects…