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We report lucky imaging observations of 62 pairs at mid-southern declinations sourced from the WDS with separations larger than 4 arc seconds and magnitude less than 10. The measures comprise separations and PA calibrated against Alpha…

太阳与恒星天体物理 · 物理学 2020-11-10 Matthew James , Rod Letchford , Graeme L White , Meg Emery , Stephen Bosi

The triple system HD158926 (lambda Sco) has been observed interferometrically with the Sydney University Stellar Interferometer and the elements of the wide orbit have been determined. These are significantly more accurate than the previous…

We present orbital elements and mass sums for eighteen visual binary stars of spectral types B to K (five of which are new orbits) with periods ranging from 20 to more than 500 yr. For two double-line spectroscopic binaries with no previous…

太阳与恒星天体物理 · 物理学 2017-10-25 Rene A. Mendez , Ruben M. Claveria , Marcos E. Orchard , Jorge F. Silva

The binary star delta Sco (HD143275) underwent remarkable brightening in the visible in 2000, and continues to be irregularly variable. The system was observed with the Sydney University Stellar Interferometer (SUSI) in 1999, 2000, 2001,…

天体物理学 · 物理学 2015-05-13 W. J. Tango , J. Davis , A. P. Jacob , A. Mendez , J. R. North , J. W. O'Byrne , E. B. Seneta , P. G. Tuthill

We present the results of 938 speckle measures of double stars and suspected double stars drawn mainly from the Hipparcos Catalogue, as well as 208 observations where no companion was noted. One hundred fourteen pairs have been resolved for…

太阳与恒星天体物理 · 物理学 2015-10-28 Elliott P. Horch , Gerard T. van Belle , James W. Davidson, , Lindsay A. Ciastko , Mark E. Everett , Karen S. Bjorkman

We derive single-epoch radial velocities for a sample of 56 B-type stars members of the subgroups Upper Scorpius, Upper Centaurus Lupus and Lower Centaurus Crux of the nearby Sco-Cen OB association. The radial velocity measurements were…

天体物理学 · 物理学 2009-11-11 E. Jilinski , S. Daflon , K. Cunha , R. de la Reza

We present orbital elements, orbital parallaxes and individual component masses, for fourteen spatially resolved double-line spectroscopic binaries derived doing a simultaneous fit of their visual orbit and radial velocity curve. This was…

太阳与恒星天体物理 · 物理学 2022-02-16 Jennifer Anguita-Aguero , Rene A. Mendez , Ruben M. Claveria , Edgardo Costa

We present photometric, astrometric, and spectroscopic observations of USco160611.9-193532 AB, a candidate ultrawide (~1600 AU), low-mass (M_tot~0.4 M_sun) multiple system in the nearby OB association Upper Scorpius. We conclude that both…

天体物理学 · 物理学 2009-09-29 Adam L. Kraus , Lynne A. Hillenbrand

We present the results of a high-resolution imaging survey of 12 brown dwarfs and very low mass stars in the closest (~145 pc) young (~5 Myr) OB association, Upper Scorpius. We obtained images with the Advanced Camera for Surveys/High…

天体物理学 · 物理学 2009-11-13 A. L. Kraus , R. J. White , L. A. Hillenbrand

We present a detailed analysis of the detached eclipsing binary system HO Telescopii, which contains two A-type stars in a circular orbit of period 1.613 d. We use light curves from the Transiting Exoplanet Survey Satellite (TESS), which…

太阳与恒星天体物理 · 物理学 2024-08-26 John Southworth

In anticipation of the possible collision between a circumstellar disk and the secondary star in the highly eccentric binary system Delta Scorpii, high angular resolution interferometric observations have been acquired aimed at revising the…

太阳与恒星天体物理 · 物理学 2015-05-27 C. Tycner , A. Ames , R. T. Zavala , C. A. Hummel , J. A. Benson , D. J. Hutter

The two main components of the closest star system, {\alpha}-Centauri AB(RA 14h39m, Dec-60o50', J2000.0) is indubitbaly one of the most studied visual double stars. This paper presents the results of our recalculation of orbital and…

地球与行星天体物理 · 物理学 2010-07-30 Suryadi Siregar , Hanindyo Kuncarayakti

Results of speckle observations at the 4.1-m SOAR telescope in 2012 (158 measures of 121 systems, 27 non-resolutions) are reported. The aim is to follow fast orbital motion of recently discovered or neglected close binaries and sub-systems.…

太阳与恒星天体物理 · 物理学 2015-06-05 Andrei Tokovinin

The first orbital solution for the spectroscopic pair in the multiple star system sigma Scorpii, determined from measurements with the Sydney University Stellar Interferometer (SUSI), is presented. The primary component is of beta Cephei…

天体物理学 · 物理学 2009-11-13 J. R. North , J. Davis , P. G. Tuthill , W. J. Tango , J. G. Robertson

The bright southern binary star beta Centauri (HR 5267) has been observed with the Sydney University Stellar Interferometer (SUSI) and spectroscopically with the ESO CAT and Swiss Euler telescopes at La Silla. The interferometric…

This paper details speckle observations of binary stars taken at the Lowell Discovery Telescope, the WIYN Telescope, and the Gemini telescopes between 2016 January and 2019 September. The observations taken at Gemini and Lowell were done…

We report on a significantly improved determination of the physical orbit of the double-lined spectroscopic binary system 12 Boo. We have a 12 Boo interferometry dataset spanning six years with the Palomar Testbed Interferometer, a smaller…

天体物理学 · 物理学 2009-11-10 Andrew F. Boden , Guillermo Torres , Christian A. Hummel

We report the detection of seven low mass companions to intermediate-mass stars (SpT B/A/F; $M$$\approx$1.5-4.5 solar masses) in the Scorpius-Centaurus Association using nonredundant aperture masking interferometry. Our newly detected…

We present measurements in the context of a survey of southern hemisphere binary and multiple stellar systems observed with the Zorro Speckle dual diffraction-limited optical imaging camera on the 8.1m Gemini-South telescope carried out…

太阳与恒星天体物理 · 物理学 2025-03-13 Rene A. Mendez , Andrei Tokovinin , Edgardor Costa , Max Dirk

We present interferometric observations of the sigma Orionis triple system using the CHARA Array, NPOI, and VLTI. Using these measurements, we spatially resolve the orbit of the close spectroscopic binary (Aa,Ab) for the first time and…

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