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相关论文: A Close Companion Search around L Dwarfs using Ape…

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This paper revisits a sample of ultracool dwarfs in the Solar neighborhood previously observed with the Hubble Space Telescope's NICMOS NIC1 instrument. We have applied a novel high angular resolution data analysis technique based on the…

太阳与恒星天体物理 · 物理学 2015-06-15 Benjamin Pope , Frantz Martinache , Peter Tuthill

The current direct observations of brown dwarfs and exoplanets have been obtained using instruments not specifically designed for overcoming the large contrast ratio between the host star and any wide-separation faint companions. However,…

天体物理仪器与方法 · 物理学 2015-06-03 Sasha Hinkley

Aims. We search for low-mass companions in the innermost region (<300 mas, i.e., 6 AU) of the beta Pic planetary system. Methods. We obtained interferometric closure phase measurements in the K-band with the VLTI/AMBER instrument used in…

We present preliminary results of an imaging survey for companions to low-luminosity dwarfs with spectral types ranging from M7 to L9. A K-band study with the Near Infrared Camera (NIRC) at the Keck telescope discriminates against…

天体物理学 · 物理学 2007-05-23 D. W. Koerner , J. Davy Kirkpatrick , I. N. Reid , J. Gizis

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,…

太阳与恒星天体物理 · 物理学 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

Extrasolar planet searches targeting very low-mass stars and brown dwarfs are hampered by intrinsic or instrumental limitations. Time series of astrometric measurements with precisions better than one milli-arcsecond can yield new evidence…

太阳与恒星天体物理 · 物理学 2014-05-08 J. Sahlmann , P. F. Lazorenko , D. Segransan , E. L. Martin , M. Mayor , D. Queloz , S. Udry

We describe a near-IR photometric search for cool red dwarf companions to hot EUV-detected white dwarfs (WDs). While some composite systems have been found optically among WDs detected in recent EUV All-Sky Surveys, we develop an IR…

天体物理学 · 物理学 2009-10-31 Paul J. Green , Babar Ali , Ralf Napiwotzki

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

We present the observational results of a near-infrared survey of a large sample of Class I protostars designed to determine the Class I binary separation distribution from ~100 AU to ~5000 AU. We have selected targets from a new sample of…

天体物理学 · 物理学 2009-11-13 Michael Connelley , Bo Reipurth , Alan Tokunaga

We present analysis of HST Planetary Camera images of twenty L dwarfs identified in the course of the Two Micron All-Sky Survey. Four of the targets have faint, red companions at separations between 0.07 and 0.29 arcseconds (1.6 to 7.6 AU).…

天体物理学 · 物理学 2010-04-06 I. Neill Reid , John E. Gizis , J. Davy Kirkpatrick , D. W. Koerner

Microlensing is sensitive to binary, brown dwarf, and planetary companions to normal stars in the Galactic bulge with separations between about 1-10 AU. The accurate, densely-sampled photometry of microlensing events needed to detect…

天体物理学 · 物理学 2007-05-23 B. Scott Gaudi

We present two confirmed wide separation L-dwarf common proper motion companions to nearby stars and one candidate identified from the Two Micron All Sky Survey. Spectral types from optical spectroscopy are L0 V, L2.5 V, and L8 V.…

天体物理学 · 物理学 2009-11-07 J. C. Wilson , J. Davy Kirkpatrick , J. E. Gizis , M. F. Skrutskie , D. G. Monet , J. R. Houck

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…

Observational data on companion statistics around young stellar systems is needed to flesh out the formation pathways for extrasolar planets and brown dwarfs. Aperture masking is a new technique that is able to address an important part of…

天体物理仪器与方法 · 物理学 2015-05-28 S. Lacour , P. Tuthill , P. Amico , M. Ireland , D. Ehrenreich , N. Huelamo , A. -M. Lagrange

We report techniques and results of a Palomar 200-inch (5 m) adaptive optics imaging survey of sub-stellar companions to solar-type stars. The survey consists of Ks coronagraphic observations of 21 FGK dwarfs out to 20 pc (median distance…

We present the results of a study to discover prospective new white dwarf-L dwarf binaries as identified by their near-infrared excesses in the UKIDSS catalogue. We obtained optical spectra to validate the white dwarf nature for 22 of the…

We present the results of an aperture masking interferometry survey for substellar companions around 67 members of the young (~8-200Myr) nearby (~5-86pc) AB Doradus, Beta Pictoris, Hercules-Lyra, TW Hya, and Tucana-Horologium stellar…

This paper presents results of a near-infrared imaging survey for low mass stellar and substellar companions to white dwarfs. A wide field proper motion survey of 261 white dwarfs was capable of directly detecting companions at orbital…

天体物理学 · 物理学 2009-11-11 J. Farihi , E. E. Becklin , B. Zuckerman

We present the results of a deep-imaging search for wide companions to low-mass stars and brown dwarfs using NSFCam on IRTF. We searched a sample of 132 M7-L8 dwarfs to magnitude limits of $J \sim 20.5$ and $K \sim 18.5$, corresponding to…

天体物理学 · 物理学 2008-11-26 Peter R. Allen , David W. Koerner , Michael W. McElwain , Kelle L. Cruz , I. Neill Reid

We report the discovery of 14 low-mass binary systems containing mid-M to mid-L dwarf companions with separations larger than 250 AU. We also report the independent discovery of 9 other systems with similar characteristics that were…

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