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Related papers: A Common Proper Motion Stellar Companion to HAT-P-…

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We report the detection of a radial velocity companion to SDSS J091709.55+463821.8, the lowest mass white dwarf currently known with M~0.17Msun. The radial velocity of the white dwarf shows variations with a semi-amplitude of 148.8 km/s and…

Multi-epoch observations with ACS on HST provide a unique and comprehensive probe of stellar dynamics within NGC 6397. We are able to confront analytic models of the globular cluster with the observed stellar proper motions. The measured…

Solar and Stellar Astrophysics · Physics 2015-06-11 J. S. Heyl , H. Richer , J. Anderson , G. Fahlman , A. Dotter , J. Hurley , J. Kalirai , R. M. Rich , M. Shara , P. Stetson , K. A. Woodley , D. Zureko

We show that the very close-by (19 pc) K0 star HD 189733, already found to be orbited by a transiting giant planet, is the primary of a double-star system, with the secondary being a mid-M dwarf with projected separation of about 216 AU…

Astrophysics · Physics 2009-11-11 Gaspar A. Bakos , Andras Pal , David W. Latham , Robert W. Noyes , Robert P. Stefanik

A global Markov Chain Monte Carlo analysis of published eclipse photometry and radial velocities is presented for the transiting planet HD 80606b. Despite the lack of a complete transit light curve, the size of the planet is measured with a…

Earth and Planetary Astrophysics · Physics 2009-06-29 M. Gillon

We report the detection of a new low-mass stellar companion to the white dwarf HIP 3678 A, the central star of the planetary nebula NGC 246. The newly found companion is located about 1 arcsec (at projected separation of about 500 au)…

Solar and Stellar Astrophysics · Physics 2014-09-19 C. Adam , M. Mugrauer

We report the discovery of HATS-2b, the second transiting extrasolar planet detected by the HATSouth survey. HATS-2b is moving on a circular orbit around a V=13.6 mag, K-type dwarf star (GSC 6665-00236), at a separation of 0.0230 \pm 0.0003…

All transiting planet observations are at risk of contamination from nearby, unresolved stars. Blends dilute the transit signal, causing the planet to appear smaller than it really is, or produce a false positive detection when the target…

Earth and Planetary Astrophysics · Physics 2015-06-16 Elisabeth R. Adams , Andrea K. Dupree , Craig Kulesa , Don McCarthy

We report on the discovery of a white dwarf companion to the nearby late G dwarf star, HD 159062. The companion is detected in 14 years of precise radial velocity (RV) data, and in high-resolution imaging observations. RVs of HD 159062 from…

We constrain the angular momentum architecture of HD 106906, a 13 $\pm$ 2 Myr old system in the ScoCen complex composed of a compact central binary, a widely separated planetary-mass tertiary HD 106906 b, and a debris disk nested between…

Earth and Planetary Astrophysics · Physics 2021-11-03 Marta L. Bryan , Eugene Chiang , Caroline V. Morley , Gregory N. Mace , Brendan P. Bowler

We report on the discovery of HAT-P-12b, a transiting extrasolar planet orbiting the moderately bright V=12.8 K4 dwarf GSC 03033-00706, with a period P = 3.2130598 +- 0.0000021 d, transit epoch Tc = 2454419.19556 +- 0.00020 (BJD) and…

We present measurements of the spin-orbit misalignments of the hot Jupiters HAT-P-41 b and WASP-79 b, and the aligned warm Jupiter Kepler-448 b. We obtained these measurements with Doppler tomography, where we spectroscopically resolve the…

Earth and Planetary Astrophysics · Physics 2017-09-20 Marshall C. Johnson , William D. Cochran , Brett C. Addison , Chris G. Tinney , Duncan J. Wright

We report a late M-type, common proper motion companion to a nearby young visual binary HIP 115147 (V368 Cep), separated by 963 arcseconds from the primary K0 dwarf. This optically dim star has been identified as a candidate high proper…

Astrophysics · Physics 2009-11-13 V. V. Makarov , N. Zacharias , G. S. Hennessy , H. C. Harris , A. K. B. Monet

Context. Detecting and characterizing substellar companions for which the luminosity, mass, and age can be determined independently is of utter importance to test and calibrate the evolutionary models due to uncertainties in their formation…

Chauvin et al. 2005 imaged a co-moving companion at ~260 AU from the young star AB Pic A. Evolutionary models predictions based on J H K photometry of AB Pic b suggested a mass of ~13 - 14 MJup, placing the object at the deuterium-burning…

Earth and Planetary Astrophysics · Physics 2015-05-14 M. Bonnefoy , G. Chauvin , P. Rojo , F. Allard , A. -M. Lagrange , D. Homeier , C. Dumas , J. -L. Beuzit

The directly detected planetary mass companion candidate close to the young, nearby star Fomalhaut is a subject of intense discussion. While the detection of common proper motion led to the interpretation as Jovian-mass companion, later…

Solar and Stellar Astrophysics · Physics 2015-06-23 Ralph Neuhaeuser , Markus Hohle , Christian Ginski , Janos Schmidt , Valeri Hambaryan , Tobias Schmidt

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 near-infrared, follow-up imaging and spectroscopic observations at VLT, aimed at characterizing the long-period companions of the exoplanet host stars HD196885, HD1237 and HD27442. The three companions were…

Astrophysics · Physics 2007-11-01 G. Chauvin , A. -M. Lagrange , S. Udry , M. Mayor

We present a large-scale, volume-limited companion survey of 245 late-K to mid-M (K7-M6) dwarfs within 15 pc. Infrared adaptive optics (AO) data were analysed from the Very Large Telescope, Subaru Telescope, Canada-France-Hawaii Telescope,…

Solar and Stellar Astrophysics · Physics 2015-06-24 K. Ward-Duong , J. Patience , R. J. De Rosa , J. Bulger , A. Rajan , S. P. Goodwin , Richard J. Parker , D. W. McCarthy , C. Kulesa

We have carried out high-precision timing observations of the eclipsing binary PSR J2051-0827 in the 3.3 years since its discovery. These data indicate that the orbital period is decreasing at a rate of dPb/dt = (-11+-1)X10^-12. If secular,…

Astrophysics · Physics 2009-10-30 B. W. Stappers , M. Bailes , R. N. Manchester , J. S. Sandhu , M. Toscano
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