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相关论文: Stellar Companions to Stars with Planets

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We have undertaken an adaptive optics (AO) imaging survey of extrasolar planetary systems and stars showing interesting radial velocity trends from high precision radial velocity searches. AO increases the resolution and dynamic range of an…

The dynamical influence of binary companions is expected to profoundly influence planetary systems. However, the difficulty of identifying planets in binary systems has left the magnitude of this effect uncertain; despite numerous…

地球与行星天体物理 · 物理学 2016-06-29 Adam L. Kraus , Michael J. Ireland , Daniel Huber , Andrew W. Mann , Trent J. Dupuy

We present results of the CFHT adaptive optics search for companions of a homogeneous group of contact binary stars, as a contribution to our attempts to prove a hypothesis that these binaries require a third star to become so close as…

天体物理学 · 物理学 2009-09-29 Slavek M. Rucinski , Theodor Pribulla , Marten van Kerkwijk

We have carried out a search for co-moving stellar and substellar companions around 18 exoplanet host stars with the infrared camera MAGIC at the 2.2m Calar Alto telescope, by comparing our images with images from the all sky surveys 2MASS,…

天体物理学 · 物理学 2009-11-11 Markus Mugrauer , R. Neuhaeuser , T. Mazeh , E. Guenther , M. Fernandez , C. Broeg

Our Keck/NIRC2 imaging survey searches for stellar companions around 144 systems with radial velocity (RV) detected giant planets to determine whether stellar binaries influence the planets' orbital parameters. This survey, the largest of…

We have performed a Keck adaptive optics (AO) imaging survey of 25 extrasolar planetary systems discovered by the radial velocity programs. Typically, the high-resolution (FWHM~0.04") near-infrared images are able to detect point sources at…

天体物理学 · 物理学 2014-10-13 K. L. Luhman , Ray Jayawardhana

We present preliminary results of a radial-velocity search for companions to a volume limited sample of M dwarfs. Typical accuracy range between 10m/s for the brighter stars and 70m/s at our limiting magnitude. We complement the radial…

天体物理学 · 物理学 2007-05-23 X. Delfosse , T. Forveille , J. -L. Beuzit , S. Udry , M. Mayor , C. Perrier

A sample of 14 pre-main sequence visual binary systems in southern star-forming regions were imaged at 2 um with the Keck I telescope to search for tertiary companions, scattered-light disks, and compact nebulae at linear scales of 5-100…

天体物理学 · 物理学 2009-11-07 C. D. Koresko

We conducted a survey of nearby binary systems composed of main sequence stars of spectral types F and G in order to improve our understanding of the hierarchical nature of multiple star systems. Using Robo-AO, the first robotic adaptive…

We present the first search for binary companions of Massive Young Stellar Objects (MYSOs) using AO-assisted $K$ band observations, with NaCo at the VLT. We have surveyed 32 MYSOs from the RMS catalogue, probing the widest companions, with…

太阳与恒星天体物理 · 物理学 2019-01-23 Robert Pomohaci , René D. Oudmaijer , Simon P. Goodwin

We present the results of a speckle interferometric survey of Galactic massive stars that complements and expands upon a similar survey made over a decade ago. The speckle observations were made with the KPNO and CTIO 4 m telescopes and…

天体物理学 · 物理学 2009-11-13 Brian D. Mason , William I. Hartkopf , Douglas R. Gies , Todd J. Henry , John W. Helsel

The results of an adaptive optics survey of exoplanet host stars for stellar companions is presented. We used the AEOS Telescope and its adaptive optics system to collect deep images of the stars in $I$-band. Sixty-two exoplanet host stars…

太阳与恒星天体物理 · 物理学 2015-05-30 Lewis C. Roberts , Nils H. Turner , Theo A. ten Brummelaar , Brian D. Mason , William I. Hartkopf

Young intermediate-mass stars have become high-priority targets for direct-imaging planet searches following the recent discoveries of planets orbiting e.g. HR 8799 and Beta Pictoris. Close stellar companions to these stars can affect the…

太阳与恒星天体物理 · 物理学 2014-08-26 Kevin Gullikson , Adam Kraus , Sarah Dodson-Robinson

Improving direct detection capability close to the star through improved star-subtraction and post-processing techniques is vital for discovering new low-mass companions and characterizing known ones at longer wavelengths. We present…

In recent decades, thousands of substellar companions have been discovered with both indirect and direct methods of detection. In this paper, we focus our attention on substellar companions detected with the direct imaging technique, with…

We present the results of a deep imaging survey of stars surrounded by planets detected with the radial velocity technique. The purpose is to search for and to characterize long-period stellar and substellar companions. The sample contains…

天体物理学 · 物理学 2009-11-11 G. Chauvin , A. -M. Lagrange , S. Udry , T. Fusco , F. Galland , D. Naef , J. -L. Beuzit , M. Mayor

We present the results of an all-sky survey made with the Fine Guidance Sensor on Hubble Space Telescope to search for angularly resolved binary systems among the massive stars. The sample of 224 stars is comprised mainly of Galactic O- and…

Binary stars constitute a large percentage of the stellar population, yet relatively little is known about the planetary systems orbiting them. Most constraints on circumbinary planets (CBPs) so far come from transit observations with the…

We present high-resolution observations of a sample of 75 K2 targets from Campaigns 1-3 using speckle interferometry on the Southern Astrophysical Research (SOAR) telescope and adaptive optics (AO) imaging at the Keck II telescope. The…

Roughly half of Solar-type planet hosts have stellar companions, so understanding how these binary companions affect the formation and evolution of planets is an important component to understanding planetary systems overall. Measuring the…

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