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Related papers: Discovery of a Wide Low-mass Binary System in Uppe…

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We present the results of a near-infrared adaptive optics survey with the aim to detect close companions to Hipparcos members in the three subgroups of the nearby OB association Sco OB2: Upper Scorpius (US), Upper Centaurus Lupus (UCL) and…

This paper presents the results of a search for brown dwarfs in the Upper Scorpius Association using data from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Cluster Survey. Candidate young brown dwarfs were first chosen by their…

Solar and Stellar Astrophysics · Physics 2015-05-30 P. Dawson , A. Scholz , T. P. Ray

We present the results of a search for wide binary systems among 783 members of three nearby young associations: Taurus-Auriga, Chamaeleon I, and two subgroups of Upper Scorpius. Near-infrared (JHK) imagery from 2MASS was analyzed to search…

Astrophysics · Physics 2011-02-11 Adam L. Kraus , Lynne A. Hillenbrand

We present the discovery of the common proper motion M9 + L0 binary DENIS J220002.05-303832.9AB, identified serendipitously with the SpeX near infrared imager/spectrograph. Spectral types are derived from resolved near infrared spectroscopy…

Astrophysics · Physics 2009-11-11 Adam J. Burgasser , Michael W. McElwain

We report the discovery of a faint L6 \pm 1 companion to the previously known M9 dwarf, 2MASS J01303563-4445411, based on our near-infrared imaging and spectroscopic observations with the 3m Infrared Telescope Facility SpeX…

Solar and Stellar Astrophysics · Physics 2012-02-10 Saurav Dhital , Adam J. Burgasser , Dagny L. Looper , Keivan G. Stassun

We report our discovery of a nearby wide binary system, LP 714-37 AB. Phan-Bao et al. identified LP 714-37 as a mid-M dwarf during a cross-identification of the NLTT and DENIS catalogues. Our CCD images resolve the system into a binary with…

Astrophysics · Physics 2009-11-13 N. Phan-Bao , E. L. Martin , C. Reyle , T. Forveille , J. Lim

We describe an astrometric and spectroscopic campaign to confirm the youth and association of a complete sample of candidate wide companions in Taurus and Upper Sco. Our survey found fifteen new binary systems (3 in Taurus and 12 in Upper…

Solar and Stellar Astrophysics · Physics 2015-05-13 Adam L. Kraus , Lynne A. Hillenbrand

We conducted a deep survey of resolved sub-systems among wide binaries with solar-type components within 67 pc from the Sun. Images of 61 stars in the K and H bands were obtained with the NICI adaptive-optics instrument on the 8-m…

Solar and Stellar Astrophysics · Physics 2015-05-19 Andrei Tokovinin , Markus Hartung , Thomas L Hayward

We report the identification of 2MASS J15500845+1455180 as a 0"9 L dwarf visual binary. This source is resolved in Sloan Digital Sky Survey (SDSS) images and in near-infrared imaging with the IRTF SpeX imager/spectrometer. The two…

Solar and Stellar Astrophysics · Physics 2014-11-20 Adam J. Burgasser , Saurav Dhital , Andrew West

We present a 3-5um LBT/MMT adaptive optics imaging study of three Upper Scorpius stars with brown dwarf (BD) companions with very low-masses/mass ratios (M_BD < 25M_Jup; M_BD / M_star ~ 1-2%), and wide separations (300-700 AU): GSC 06214,…

We have obtained high contrast images of four nearby, faint, and very low mass objects 2MASSJ04351455-1414468, SDSSJ044337.61+000205.1, 2MASSJ06085283-2753583 and 2MASSJ06524851-5741376 (here after 2MASS0435-14, SDSS0443+00, 2MASS0608-27…

We present the results of a radial velocity (RV) survey of 14 brown dwarfs (BDs) and very low-mass (VLM) stars in the Upper Scorpius OB association (UScoOB) and 3 BD candidates in the rho Ophiuchi dark cloud core. We obtained…

Astrophysics · Physics 2009-11-11 Ryuichi Kurosawa , Tim J. Harries , S. P. Littlefair

We present 4.5, 8, and 16um photometry from the Spitzer Space Telescope for 204 stars in the Upper Scorpius OB Association. The data are used to investigate the frequency and properties of circumstellar disks around stars with masses…

Astrophysics · Physics 2011-02-11 John M. Carpenter , Eric E. Mamajek , Lynne A. Hillenbrand , Michael R. Meyer

Free-floating planetary mass objects--worlds that roam interstellar space untethered to a parent star--challenge conventional notions of planetary formation and migration, but also of star and brown dwarf formation. We focus on the…

We present the discoveries of three faint companions to young stars in the Scorpius-Centaurus region, imaged with the NICI instrument on Gemini South. We have confirmed all three companions through common proper motion tests. Follow-up…

Solar and Stellar Astrophysics · Physics 2015-06-11 Markus Janson , Ray Jayawardhana , Julien H. Girard , David Lafreniere , Mariangela Bonavita , John Gizis , Alexis Brandeker

The triple system HD158926 (lambda Sco) has been observed interferometrically with the Sydney University Stellar Interferometer and the elements of the wide orbit have been determined. These are significantly more accurate than the previous…

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 report on the results of a survey for radial velocity variability in a heterogeneous sample of very low-mass stars and brown dwarfs. One distinguishing characteristic of the survey is its timespan, which allows an overlap between…

Astrophysics · Physics 2008-11-26 Gibor Basri , Ansgar Reiners

We present observations of three protoplanetary disks in visible scattered light around M-type stars in the Upper Scorpius OB association using the STIS instrument on the Hubble Space Telescope. The disks around stars 2MASS…

Earth and Planetary Astrophysics · Physics 2021-04-28 Samuel Walker , Maxwell Millar-Blanchaer , Bin Ren , Paul Kalas , John Carpenter

We analyze Spitzer IRS spectra of 110 B-, A-, F-, and G-type stars with optically thin infrared excess in the Scorpius-Centaurus (ScoCen) OB association. The age of these stars ranges from 11-17 Myr. We fit the infrared excesses observed in…

Earth and Planetary Astrophysics · Physics 2015-07-24 Hannah Jang-Condell , Christine H. Chen , Tushar Mittal , P. Manoj , Dan Watson , Carey M. Lisse , Erika Nesvold , Marc Kuchner