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相关论文: Absolute Proper Motions of Open Clusters: I. Obser…

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We have identified 317 stars included in the Hipparcos astrometric catalogue which have parallaxes measured to a precision of better than 15%, and whose location in the (M_V, (B-V)_T) diagram implies a metallicity comparable to or less than…

天体物理学 · 物理学 2009-10-31 I. Neill Reid , F. van Wyk , F. Marang , G. Roberts , D. Kilkenny , S. Mahoney

In this study, we investigate the fundamental astrophysical parameters of the old open cluster NGC 188 through two complementary methods: isochron-fitting and spectral energy distribution (SED) analysis. Using photometric, astrometric, and…

星系天体物理 · 物理学 2024-12-11 Deniz Cennet Dursun , Seval Taşdemir , Seliz Koç , Srishti İyer

We determined the cluster apex coordinates, studied the substructures and performed membership analysis in the central part (34'X33') of the open cluster M 67. We used the individual stellar apexes method developed earlier and classical…

星系天体物理 · 物理学 2015-06-19 S. V. Vereshchagin , N. V. Chupina , Devesh P. Sariya , R. K. S. Yadav , Brijesh Kumar

We present a pilot study of Galactic globular cluster (GC) proper motion (PM) determinations using Gaia data. We search for GC stars in the Tycho-Gaia Astrometric Solution (TGAS) catalogue from Gaia Data Release 1 (DR1), and identify five…

太阳与恒星天体物理 · 物理学 2017-06-22 Laura L. Watkins , Roeland P. van der Marel

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

We present a new procedure for the identification of moving groups. It is a combination of two independent member selection methods. One is a modern implementation of a classical convergent point method for proper motion data. The other…

天体物理学 · 物理学 2007-05-23 J. H. J. de Bruijne , R. Hoogerwerf , A. G. A. Brown , L. A. Aguilar , P. T. de Zeeuw

WFPC2 images obtained with the Hubble Space telescope 4.16 years apart have allowed us to measure the proper motion of the metal rich globular cluster NGC 6553 with respect to the background bulge stars. With a space velocity of (${\Pi},…

天体物理学 · 物理学 2016-01-27 M. Zoccali , A. Renzini , S. Ortolani , E. Bica , B. Barbuy

We have conducted a systematic search for high proper motion stars in the Digitized Sky Survey, in the area of the sky north of -2.8 degrees in declination and within 25 degrees of the galactic plane. Using the SUPERBLINK software, a…

天体物理学 · 物理学 2011-03-28 Sebastien Lepine , Michael M. Shara , R. Michael Rich

A new method for the determination of open cluster membership based on a cumulative effect is proposed. In the field of a plate the relative x and y coordinate positions of each star with respect to all the other stars are added. The…

天体物理学 · 物理学 2010-02-18 G. Javakhishvili , V. Kukhianidze , M. Todua , R. Inasaridze

We have measured the absolute proper motions of globular clusters NGC 2808, 3201, 4372, 4833, 5927 and 5986. The proper motions are on the Hipparcos system and they are the first determinations ever made for these low Galactic latitude…

天体物理学 · 物理学 2009-06-23 D. I. Casetti-Dinescu , T. M. Girard , D. Herrera , W. F. van Altena , C. E. López , D. J. Castillo

New estimate of the distances of 36 nearby galaxies is presented. It is based on the calibration of the V- and I-band Period-Lumi- nosity relations for galactic Cepheids measured by the HIPPARCOS mission. The distance moduli are obtained in…

天体物理学 · 物理学 2009-11-07 G. Paturel , P. Teerikorpi , G. Theureau , P. Fouque , I. Musella , J. N. Terry

The results of astrometric and photometric investigations of the open cluster NGC 7243 are presented. Proper motions of 2165 stars with root-mean-square error of 1.1 mas/yr were obtained by means of PDS scanning of astrometric plates…

天体物理学 · 物理学 2009-11-07 E. G. Jilinski , V. N. Frolov , J. K. Ananjevskaja , J. Straume , N. A. Drake

A sample of subdwarfs with accurate space velocities and standarized metallicities is presented. This was constructed by combining Hipparcos parallaxes ond proper motions with radial velocities and metallicities from Carney et al. (1994;…

天体物理学 · 物理学 2009-10-31 B. Fuchs , H. Jahreiss , R. Wielen

The Hipparcos proper motions of 220 galactic Cepheids, together with relevant ground-based photometry, have been analysed. The effects of galactic rotation are very clearly seen. Mean values of the Oort constants, A = 14.82 +/- 0.84…

天体物理学 · 物理学 2015-06-24 Michael Feast , Patricia Whitelock

We introduce a new kinematic method to investigate the structure of open star clusters. We adopt a hierarchical clustering algorithm that uses the celestial coordinates and the proper motions of the stars in the field of view of the cluster…

星系天体物理 · 物理学 2020-08-26 Heng Yu , Zheng-Yi Shao , Antonaldo Diaferio , Lu Li

We use proper motion measurements to determine the real size and membership richness of a sample of open clusters located at high galactic latitudes (40 < |b| < 90).

天体物理学 · 物理学 2009-06-25 A. L. Tadross

We present a study of 7 southern open clusters based on UBVRI CCD photomety (Johnsons-Cousins system) and Gaia DR2 data. Dias 4, Dias 6 and four other clusters had UBVRI photometric observations determined for the first time. From the…

太阳与恒星天体物理 · 物理学 2018-09-05 Wilton S. Dias , Hektor Monteiro , Jacques R. D. Lépine , R. Prates , C. D. Gneiding , M. Sacchi

We present a catalog of 1147 candidate common proper motion binaries selected from the revised New Luyten Two-Tenths Catalog. Among these, we identify 999 genuine physical pairs using the measured proper-motion difference and the relative…

天体物理学 · 物理学 2009-11-10 Julio Chaname , Andrew Gould

We present a list of 130 Galactic Open Clusters, found in the All-Sky Compiled Catalogue of 2.5 Million Stars (ASCC-2.5). For these clusters we determined and publish a homogeneous set of astrophysical parameters such as size, membership,…

天体物理学 · 物理学 2016-08-16 N. V. Kharchenko , A. E. Piskunov , S. Röser , E. Schilbach , R. -D. Scholz

We have determined possible cluster members of the nearby open cluster Praesepe (M44) based on J and K photometry and proper motions from the PPMXL catalogue and z photometry from the Sloan Digital Sky Survey (SDSS). In total we identified…

星系天体物理 · 物理学 2013-07-09 Pouria Khalaj , Holger Baumgardt