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Related papers: UrHip Proper Motion Catalog

200 papers

Accelerations of both the solar system barycenter (SSB) and stars in the Milky Way cause a systematic observational effect on the stellar proper motions, which was first studied in the early 1990s and developed by J. Kovalevsky (aberration…

Astrophysics of Galaxies · Physics 2015-06-16 Jia-Cheng Liu , Yi Xie , Zi Zhu

Orbits of 55 visual binary stars are computed using recent speckle interferometry data from the SOAR telescope: 33 first-time orbits and 22 revisions of previous orbit calculations. The orbital periods range from 1.4 to 370 years, the…

Solar and Stellar Astrophysics · Physics 2016-08-04 Andrei Tokovinin

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…

Solar and Stellar Astrophysics · Physics 2015-06-15 Andrei Tokovinin , Markus Hartung , Thomas L. Hayward

The combination of ground-based astrometric compilation catalogues, such as the FK5 or the GC, with the results of the ESA Astrometric Satellite HIPPARCOS produces for many thousands of stars proper motions which are significantly more…

Astrophysics · Physics 2009-10-31 R. Wielen , H. Lenhardt , H. Schwan , C. Dettbarn

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.…

Solar and Stellar Astrophysics · Physics 2015-06-05 Andrei Tokovinin

We use 14-year baseline images obtained with the Wide Field Planetary Camera 2 on board the Hubble Space telescope to derive a proper motion for one of the Milky Way's most distant dwarf spheroidal companions, Leo II, relative to an…

Astrophysics of Galaxies · Physics 2015-05-30 Sébastien Lépine , Andreas Koch , R. Michael Rich , Konrad Kuijken

Occultations of stars brighter than 15m by largest TNOs are predicted. Search was performed using the following catalogues: Hipparcos; Tycho2 with coordinates of 2838666 stars taken from UCAC2 (Herald, 2003); UCAC2 (Zacharias et al., 2003)…

Astrophysics · Physics 2009-11-10 Denis Denissenko

New astrometric reductions of the US Naval Observatory CCD Astrograph Catalog (UCAC) all-sky observations were performed from first principles using the TGAS stars in the 8 to 11 magnitude range as reference star catalog. Significant…

Instrumentation and Methods for Astrophysics · Physics 2017-03-29 Norbert Zacharias , Charlie Finch , Julien Frouard

We have derived a new photographic photometry and proper motions for 20000 stars with completeness to V = 18 in the direction of galactic center at the intermediate latitude (l = 3 deg,b = 47 deg; alpha(1950)=15h 18m, delta(1950) = +02deg…

Astrophysics · Physics 2007-05-23 D. K. Ojha , O. Bienayme , A. C. Robin , V. Mohan

We present the results of our 2nd radial velocity monitoring campaign, carried out with the \'Echelle spectrograph FLECHAS at the University Observatory Jena in the course of the Gro{\ss}schwabhausen binary survey between December 2016 and…

Solar and Stellar Astrophysics · Physics 2020-03-04 T. Heyne , M. Mugrauer , R. Bischoff , D. Wagner , S. Hoffmann , O. Lux , V. Munz , M. Geymeier , R. Neuhäuser

We search for stars with proper motions in a set of twenty deep Subaru images, covering about 0.28 square degrees to a depth of i ~ 25, taken over a span of six years. In this paper, we describe in detail our reduction and techniques to…

Proper motions for several Milky Way dwarf spheroidal (dSph) galaxies have been determined using both ground and space-based imaging. These measurements require long baselines and repeat observations and typical errors are of order ten…

Astrophysics · Physics 2009-11-13 Manoj Kaplinghat , Louis E. Strigari

We develop Bayesian statistical methods for discovering and assigning probabilities to non-random (e.g., physical) stellar companions. These companions are either presently bound or were previously bound. The probabilities depend on…

Astrophysics of Galaxies · Physics 2015-05-19 Ed Shaya , Rob Olling

Hipparcos Intermediate Astrometric Data (IAD) have been used to derive astrometric orbital elements for spectroscopic binaries from the newly released Ninth Catalogue of Spectroscopic Binary Orbits (SB9). Among the 1374 binaries from SB9…

Astrophysics · Physics 2009-11-11 S. Jancart , A. Jorissen , C. Babusiaux , D. Pourbaix

The proper motion measurements for 143 previously known L and T dwarfs are presented. From this sample we identify and discuss 8 high velocity L dwarfs. We also find 4 new wide common proper motion binaries/multiple systems. Using the…

Data on the multiplicity of F- and G-type dwarf stars within 67pc of the Sun are presented. This distance-limited sample based on the Hipparcos catalog contains 4847 primary stars (targets) with 0.5<V-I_C<0.8 and is >90% complete. There are…

Solar and Stellar Astrophysics · Physics 2015-06-18 Andrei Tokovinin

CONTEXT.The first Gaia Data Release (DR1) significantly improved the previously available proper motions for the majority of the Tycho-2 stars. AIMS. We want to detect runaway stars using Gaia DR1 proper motions and compare our results with…

We consider two previously studied samples of OB stars with different distance scales. The first one consists of 98 massive spectroscopic binary stars with photometric distances, and the second one consists on 140 OB stars with the…

Astrophysics of Galaxies · Physics 2017-03-22 V. V. Bobylev , A. T. Bajkova

We describe a homogeneous catalog compilation of common proper motion stars based on Gaia DR2. A preliminary list of all pairs of stars within the radius of 100 pc around the Sun with a separation less than a parsec was compiled. Also, a…

Solar and Stellar Astrophysics · Physics 2020-12-16 S. A. Sapozhnikov , D. A. Kovaleva , O. Yu. Malkov , A. Yu. Sytov

Long-period companions are detected and characterized thanks to long-baseline radial velocity surveys. Combining Doppler time-series with astrometry, and in particular with proper motion anomalies technique, it is possible to put strong…

Earth and Planetary Astrophysics · Physics 2026-03-11 G. Piccinini , A. Petralia , A. Sozzetti , S. Benatti , D. Gandolfi , G. Micela