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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

Using the near-infrared spectrometer SpeX and its slit-viewing camera at the IRTF, I have resolved a low-mass member of the Upper Scorpius OB association into a double star. From K-band images of the pair, DENIS-P J161833.2-251750.4 A and…

Astrophysics · Physics 2009-11-13 K. L. Luhman

Hot subdwarf binaries with white dwarf companions with orbital periods of less than two hours are progenitor candidates for massive single white dwarfs as well as a variety of thermonuclear explosions. Our aim is to determine the binary…

We have discovered that the extremely red, low-gravity L7 dwarf 2MASS J11193254-1137466 is a 0.14" (3.6 AU) binary using Keck laser guide star adaptive optics imaging. 2MASS J11193254-1137466 has previously been identified as a likely…

Solar and Stellar Astrophysics · Physics 2017-11-10 William M. J. Best , Michael C. Liu , Trent J. Dupuy , Eugene A. Magnier

We report the discovery of a stripped giant + lower giant binary, 2M04123153+6738486 (2M0412), identified during a search for non-interacting compact object-star binaries. 2M0412 is an evolved ($T_{\rm eff, giant}\simeq4000$ K), luminous…

We exploit the precise parallaxes and proper motions contained in Gaia Data Release 2 (DR2) to establish whether the proposed wide-separation companions to five nearby, young stars are in fact equidistant and comoving with these stars. For…

Solar and Stellar Astrophysics · Physics 2018-07-30 Joel H. Kastner

We report the identification of a very low mass new binary system 2MASS J10274572+0629104, based on Kepler K2 photometry and Gaia DR2 astrometry. The K2 light curve is consistent with a beat pattern of two periodic signals, and using…

Solar and Stellar Astrophysics · Physics 2019-04-24 Rishi R. Paudel , John E. Gizis , Adam J. Burgasser , Chih-Chun Hsu

WISE J104915.57$-$531906.1 is a L/T brown dwarf binary located 2pc from the Sun. The pair contains the closest known brown dwarfs and is the third closest known system, stellar or sub-stellar. We report comprehensive follow-up observations…

We report the discovery of a substellar-mass co-moving companion to 2MASS J22501512+2325342, an M3 candidate member of the young (130--200 Myr) AB Doradus Moving Group (ABDMG). This L3 beta companion was discovered in a 2MASS search for…

Solar and Stellar Astrophysics · Physics 2018-01-10 Marie-Eve Desrochers , Etienne Artigau , Jonathan Gagné , René Doyon , Lison Malo , Jacqueline K. Faherty , David Lafrenière

2MASS J03202839-0446358AB is a recently identified, late-type M dwarf/T dwarf spectroscopic binary system for which both the radial velocity orbit for the primary and spectral types for both components have been determined. By combining…

Solar and Stellar Astrophysics · Physics 2009-11-13 Adam J. Burgasser , Cullen H. Blake

Almost all massive stars have bound stellar companions, existing in binaries or higher-order multiples. While binarity is theorized to be an essential feature of how massive stars form, essentially all information about such properties is…

[not part of Research Note] We report the discovery of a widely-separated low-mass binary as a candidate member of the $\sim$40 Myr Argus Association. Resolved imaging and astrometry with 2MASS and LDSS-3 reveal a common proper motion pair…

Solar and Stellar Astrophysics · Physics 2017-12-05 Adam J. Burgasser , Dagny L. Looper , J. Davy Kirkpatrick

A sample of bright contact binary stars (W UMa-type or EW, and related: with beta Lyr light curves, EB, and ellipsoidal, ELL - in effect, all but the detached, EA), to the limit of Vmax = 7.5 magnitude is deemed to include all discoverable…

Astrophysics · Physics 2009-11-07 Slavek M. Rucinski

Low-mass and brown dwarfs have recently been found as wide companions to many nearby stars, formerly believed to be single. Wide binaries are usually found as common proper motion pairs. Sometimes, more than two objects share the same large…

Astrophysics · Physics 2016-08-16 R. -D. Scholz , N. Lodieu , R. Ibata , O. Bienaymé , M. Irwin , M. J. McCaughrean , A. Schwope

We report the discovery of two binary systems, each consisting of a slightly bloated G-type main-sequence star and an unseen companion, identified through photometric data from TESS and radial velocity variation from Gaia. High-resolution…

We report the detection of radio emission and orbital motion from the nearby star-brown dwarf binary WISE J072003.20-084651.2AB. Radio observations across the 4.5-6.5 GHz band with the Very Large Array identify at the position of the system…

Solar and Stellar Astrophysics · Physics 2015-08-27 Adam J. Burgasser , Carl Melis , Jacob Todd , Christopher R. Gelino , Gregg Hallinan , Daniella Bardalez Gagliuffi

We present observations of a new very low mass field binary, discovered during an infrared imaging survey of 250 DENIS L and very late-M dwarfs. DENIS-J055146.0-443412.2 is an M8.5+L0 pair, with a physical separation of over 200 AU. This…

Astrophysics · Physics 2009-11-11 M. Billeres , X. Delfosse , J. -L. Beuzit , T. Forveille , L. Marchal , E. L. Martin

We report the initial results of a VLT/NACO high spatial resolution imaging survey for multiple systems among 58 M-type members of the nearby Upper Scorpius OB association. Nine pairs with separations below 100 have been resolved. Their…

We report the discovery of a brown dwarf companion to the young M dwarf 1RXS J235133.3+312720 as part of a high contrast imaging search for planets around nearby young low-mass stars with Keck-II/NIRC2 and Subaru/HiCIAO. The 2.4" (~120 AU)…

Solar and Stellar Astrophysics · Physics 2015-06-05 Brendan P. Bowler , Michael C. Liu , Evgenya L. Shkolnik , Trent J. Dupuy , Lucas A. Cieza , Adam L. Kraus , Motohide Tamura

We present the result of a systematic search for spectrally hard and soft X-ray binary systems in the Small Magellanic Cloud (SMC). This search has been applied to ROSAT PSPC data (0.1-2.4 keV) collected during 9 pointed observations…

Astrophysics · Physics 2007-05-23 P. Kahabka , W. Pietsch