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Related papers: The orbit of the brown dwarf binary Gl 569B

200 papers

Context: So far more than 60 substellar companions have been discovered around giant stars. These systems present physical and orbital properties that contrast to those detected orbiting less evolved stars. Aims: We are conducting a radial…

Earth and Planetary Astrophysics · Physics 2014-12-10 M. I. Jones , J. S. Jenkins , P. Rojo , C. H. F. Melo , P. Bluhm

We report our discovery of an extremely rare, low mass, quadruple-lined spectroscopic binary BD-22 5866 (=NLTT 53279, integrated spectral type = M0 V), found during an ongoing search for the youngest M dwarfs in the solar neighborhood. From…

We report the discovery of a widely separated (258$\farcs3\pm0\farcs$4) T dwarf companion to the Gl 570ABC system. This new component, Gl 570D, was initially identified from the Two Micron All Sky Survey (2MASS). Its near-infrared spectrum…

With an orbital period of about 3.078 days, the double-lined spectroscopic binary HD 48099 is, still now, the only short-period O+O system known in the Mon OB2 association. Even though an orbital solution has already been derived for this…

Solar and Stellar Astrophysics · Physics 2014-11-20 L. Mahy , G. Rauw , F. Martins , Y. Naze , E. Gosset , M. De Becker , H. Sana , P. Eenens

Multiple-epoch, multicolor images of the astrometric binary Gliese 105A and its very low mass companion Gliese 105C have been obtained using the Hubble Space Telescope's Wide Field Planetary Camera 2 (WFPC2) and Near-Infrared Camera and…

We have carried out high angular resolution near-infrared imaging and low-resolution (R~1000) spectroscopy of the nearest known brown dwarf, Eps Indi B, using the ESO VLT NAOS/CONICA adaptive optics system. We find it to be a close binary…

We report the discovery of a bright, brown dwarf companion to the star HIP 64892, imaged with VLT/SPHERE during the SHINE exoplanet survey. The host is a B9.5V member of the Lower-Centaurus-Crux subgroup of the Scorpius Centaurus OB…

We present the first measurement of the sky-projected orbital obliquity of a benchmark transiting brown dwarf host, HIP 33609, as a part of the Orbital Architectures of Transiting Massive Exoplanets And Low-mass stars (OATMEAL) survey. HIP…

We have found that the white dwarf PG 1101+364 is a double-lined white dwarf/white dwarf binary with an orbital period of 3.47 hours. PG 1101+364 is the shortest period detached double-degenerate yet found and gravitational radiation will…

Astrophysics · Physics 2016-06-08 T. R. Marsh

We present comprehensive orbital analyses and dynamical masses for the substellar companions Gl~229~B, Gl~758~B, HD~13724~B, HD~19467~B, HD~33632~Ab, and HD~72946~B. Our dynamical fits incorporate radial velocities, relative astrometry, and…

Using high-contrast imaging with the SPHERE instrument at the VLT, we report the first images of a cold brown dwarf companion to the exoplanet host star HD4113A. The brown dwarf HD4113C is part of a complex dynamical system consisting of a…

Earth and Planetary Astrophysics · Physics 2018-06-13 A. Cheetham , D. Ségransan , S. Peretti , J. -B. Delisle , J. Hagelberg , J-L. Beuzit , T. Forveille , M. Marmier , S. Udry , F. Wildi

We report the discovery of a wide (approximately 400 AU projected separation), common proper motion companion to the nearby M dwarf LHS 2803 (PSO J207.0300-13.7422). This object was discovered during our census of the local T dwarf…

We present the results of a spectroscopic and photometric analysis of HD314884, a slowly pulsating B star (SPB) in a binary system with detected soft X-ray emission. We spectrally classify the B star as a B5V-B6V star with T$_{eff}$ =…

Solar and Stellar Astrophysics · Physics 2015-06-22 Christopher B. Johnson , R. I. Hynes , T. Maccarone , C T. Britt , H. Davis , P. G. Jonker , M. A. P. Torres , D. Steeghs , S. Greiss , G. Nelemans

We have performed RV monitoring of the components of the binary system HD 106515 over about 11 years using the high resolution spectrograph SARG at TNG. The primary shows long-period radial velocity variations that indicate the presence of…

Earth and Planetary Astrophysics · Physics 2015-06-11 S. Desidera , R. Gratton , E. Carolo , A. F. Martinez Fiorenzano , M. Endl , D. Mesa , M. Cecconi , R. Claudi , R. Cosentino , S. Scuderi , A. Sozzetti , A. Zurlo

We have used spectra taken between 1992 and 1997 to derive the spectroscopic orbit of the eclipsing double-lined spectroscopic binary HD 197770. This binary has a period of 99.69 +/- 0.02 days and K amplitudes of 31.2 +/- 0.8 and 47.1 +/-…

Located at ~2pc, the L7.5+T0.5 dwarfs system WISE J104915.57-531906.1 (Luhman16AB) is the third closest system known to Earth, making it a key benchmark for detailed investigation of brown dwarf atmospheric properties, thermal evolution,…

Solar and Stellar Astrophysics · Physics 2017-07-05 L. R. Bedin , D. Pourbaix , D. Apai , A. J. Burgasser , E. Buenzli , H. M. J. Boffin , M. Libralato

We demonstrate that the previously identified L/T transition brown dwarf SDSS J213154.43-011939.3 (SDSS 2131-0119) is a widely separated (82.3'', $\sim$3830 au) common proper motion companion to the low-mass star NLTT 51469, which we reveal…

Solar and Stellar Astrophysics · Physics 2019-05-22 B. Gauza , V. J. S. Béjar , A. Pérez-Garrido , N. Lodieu , R. Rebolo , M. R. Zapatero Osorio , B. Pantoja , S. Velasco , J. S. Jenkins

Rotational modulations of brown dwarfs have recently provided powerful constraints on the properties of ultra-cool atmospheres, including longitudinal and vertical cloud structures and cloud evolution. Furthermore, periodic light curves…

Earth and Planetary Astrophysics · Physics 2016-03-09 Yifan Zhou , Daniel Apai , Glenn Schneider , Mark S. Marley , Adam P. Showman

We present the analysis of MOA-2007-BLG-197Lb, the first brown dwarf companion to a Sun-like star detected through gravitational microlensing. The event was alerted and followed-up photometrically by a network of telescopes from the PLANET,…

We report on nine wide common proper motion systems containing late-type M, L, or T companions. We confirm six previously reported companions, and identify three new systems. The ages of these systems are determined using diagnostics for…

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