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相关论文: Parallactic Motion for Companion Discovery: An M-D…

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We report the detection of a faint stellar companion to the famous nearby A5V star Alcor (80 UMa). The companion has M-band ($\lambda$ = 4.8 $\mu$m) magnitude 8.8 and projected separation 1".11 (28 AU) from Alcor. The companion is most…

太阳与恒星天体物理 · 物理学 2015-05-14 Eric E. Mamajek , Matthew A. Kenworthy , Philip M. Hinz , Michael R. Meyer

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…

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 present near-infrared parallax and proper motion astrometry for 74 L-dwarfs and 99 T-dwarfs, as single objects or in binary systems, obtained with the ASTROCAM astrometric imager on the USNO, Flagstaff Station 1.55-m telescope over two…

Hipparcos astrometric binaries were observed with the NICI adaptive optics system at Gemini-S, completing the work of Paper I (Tokovinin et al. 2012). Among the 65 F, G, K dwarfs within 67pc of the Sun studied here, we resolve 18 new…

太阳与恒星天体物理 · 物理学 2015-06-15 Andrei Tokovinin , Markus Hartung , Thomas L. Hayward

Observations of low-mass companions for which the dynamical masses are well constrained help to improve the calibration of evolutionary models. Such observations thereby provide more confidence in the estimation of the mass of a companion…

天体物理学 · 物理学 2009-11-13 A. Boccaletti , G. Chauvin , P. Baudoz , J. -L. Beuzit

Astrometric measurements are presented for seven nearby stars with previously detected planets: six M dwarfs (GJ 317, GJ 667C, GJ 581, GJ 849, GJ 876, and GJ 1214) and one K dwarf (BD $-$10 3166). Measurements are also presented for six…

We present preliminary results from a coronagraphic survey of young nearby Sun-like stars using the Palomar and Keck adaptive optics systems. We have targeted 251 solar analogs (F5-K5) at 20-160 pc from the Sun, spanning the 3-3000 Myr age…

天体物理学 · 物理学 2015-06-10 Stanimir Metchev , Lynne Hillenbrand

We conducted multi-epoch VLBI observations to search for astrometric reflex motion caused by a sub-stellar companion of the M8.5 dwarf TVLM 513-46546. The observations yield an absolute parallax corresponding to a distance of 10.762+/-0.027…

地球与行星天体物理 · 物理学 2015-06-16 Jan Forbrich , Edo Berger , Mark J. Reid

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

Little is known about the existence of extrasolar planets around ultracool dwarfs. Furthermore, binary stars with Sun-like primaries and very low-mass binaries composed of ultracool dwarfs show differences in the distributions of mass ratio…

太阳与恒星天体物理 · 物理学 2015-06-16 J. Sahlmann , P. F. Lazorenko , D. Segransan , E. L. Martin , D. Queloz , M. Mayor , S. Udry

Neuhaeuser et al. (2005) presented direct imaging evidence for a sub-stellar companion to the young T Tauri star GQ Lup. Common proper motion was highly significant, but no orbital motion was detected. Faint luminosity, low gravity, and a…

天体物理学 · 物理学 2009-11-13 Ralph Neuhaeuser , Markus Mugrauer , Andreas Seifahrt , Tobias Schmidt , Nikolaus Vogt

We explored the regions within a radius of 25 arcsec around 473 nearby, low-metallicity G- to M-type stars using (VR)I optical filters and small-aperture telescopes. About 10% of the sample was searched up to angular separations of 90…

天体物理学 · 物理学 2009-11-10 M. R. Zapatero Osorio , E. L. Martin

We present the first results of a multi-year program to map the orbits of M dwarf multiples within 25 parsecs. The observations were conducted primarily during 2019 - 2020 using speckle interferometry at the Southern Astrophysical Research…

太阳与恒星天体物理 · 物理学 2022-03-30 Eliot Halley Vrijmoet , Andrei Tokovinin , Todd J. Henry , Jennifer G. Winters , Elliott Horch , Wei-Chun Jao

We present a carefully vetted equatorial ($\pm$ 30$^\circ$ Decl.) sample of all known single (within 4'') mid M-dwarfs (M2.5V-M8.0V) extending out to 10 pc; their proximity and low masses make them ideal targets for planet searches. For…

We present results from an adaptive optics survey for substellar and stellar companions to Sun-like stars. The survey targeted 266 F5-K5 stars in the 3Myr to 3Gyr age range with distances of 10-190pc. Results from the survey include the…

天体物理学 · 物理学 2009-11-13 Stanimir Metchev , Lynne Hillenbrand

We report the discovery of a nearby M5.0V dwarf at 24.6 pc, SCR 1848-6855, that is orbited by an unusual companion causing an astrometric perturbation of more than 200 milli-arcseconds. This is by far the largest perturbation found to date…

太阳与恒星天体物理 · 物理学 2015-06-17 Wei-Chun Jao , Todd J. Henry , John P. Subasavage , Jennifer G. Winters , Douglas R. Gies , Adric R. Riedel , Philip A. Ianna

We present the first results from the Southern Infrared Proper Motion Survey. Using 2 Micron All Sky Survey data along with that of the SuperCOSMOS sky survey we have been able to produce the first widefield infrared proper motion survey.…

天体物理学 · 物理学 2009-11-10 N. R. Deacon , N. C. Hambly , J. A. Cooke

The knowledge of the binary properties of metal-poor and solar-metallicity stars can shed light on the potential differences between the formation processes responsible for both types of objects. The aim of the project is to determine the…

星系天体物理 · 物理学 2015-05-13 N. Lodieu , M. R. Zapatero Osorio , E. L. Martin

We perform a search for faint, common proper motion companions of Hipparcos stars using the recently published LSPM-north catalog of stars with proper motion mu>0.15 arcsec/yr. Our survey uncovers a total of 521 systems with angular…

天体物理学 · 物理学 2008-11-26 Sebastien Lepine , Bethany Bongiorno
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