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

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We present absolute trigonometric parallaxes and relative proper motions for three members of the Pleiades star cluster, obtained with HST's Fine Guidance Sensor 1r, a white-light interferometer. We estimate spectral types and luminosity…

We derive relative proper motions of stars in the fields of the globular clusters M12, NGC 6362, M4, M55, M22, NGC 6752, NGC 3201, M30, M10, NGC 362, M5, and 47 Tucanae based on data collected between 1997 and 2015 with the 1-m Swope…

太阳与恒星天体物理 · 物理学 2017-08-09 W. Narloch , J. Kaluzny , R. Poleski , M. Rozyczka , W. Pych , I. B. Thompson

Radial motions of stars in nearby moving clusters are determined from accurate proper motions and trigonometric parallaxes, without any use of spectroscopy. Assuming that cluster members share the same velocity vector (apart from a random…

天体物理学 · 物理学 2009-11-07 S. Madsen , D. Dravins , L. Lindegren

We present a study of the membership of the Hyades open cluster, derive kinematically-modelled parallaxes of its members, and study the colour-absolute magnitude diagram of the cluster. We use Gaia DR1 Tycho-Gaia Astrometric Solution (TGAS)…

星系天体物理 · 物理学 2018-04-04 Stella Reino , Jos de Bruijne , Eleonora Zari , Francesca d'Antona , Paolo Ventura

We have calculated proper motions and re-evaluated the membership probabilities of 810 stars in the area of two NGC objects, NGC 1817 and NGC 1807. We have obtained absolute proper motions from 25 plates in the reference system of the…

天体物理学 · 物理学 2009-11-10 L. Balaguer-Nunez , C. Jordi , D. Galadi-Enriquez , J. L. Zhao

Context. Selecting a cluster in proper motion space is an established method for identifying members of a star forming region. The first data release from Gaia (DR1) provides an extremely large and precise stellar catalogue, which when…

太阳与恒星天体物理 · 物理学 2018-10-10 Sam Wilkinson , Bruno Merín , Pablo Riviere-Marichalar

We present a catalog of over 6.2 million stars with measured proper motions. All these stars are observed in the direction of the Magellanic Clouds within the brightness range 12 < I < 19 mag. Based on these proper motions about 440 000…

星系天体物理 · 物理学 2012-04-26 R. Poleski , I. Soszyński , A. Udalski , M. K. Szymański , M. Kubiak , G. Pietrzyński , Ł. Wyrzykowski , K. Ulaczyk

The Hipparcos data allow a major step forward in the research of `moving groups' in the Solar neighbourhood, as the common motion of group members causes converging proper motions. Previous knowledge on these coherent structures in velocity…

天体物理学 · 物理学 2015-06-24 Jos H. J. de Bruijne

AIMS: In their 1st extension to the Milky Way Star Clusters (MWSC) survey, Schmeja et al. applied photometric filters to the 2MASS to find new cluster candidates that were subsequently confirmed or rejected by the MWSC pipeline. To further…

太阳与恒星天体物理 · 物理学 2015-09-02 R. -D. Scholz , N. V. Kharchenko , A. E. Piskunov , S. Röser , E. Schilbach

We present a catalogue of astrophysical data of 520 Galactic open clusters. These are the clusters, for which at least three most probable members (18 on average) could be identified in the ASCC-2.5, a catalogue of stars based on the…

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

Using astrometric techniques developed by Anderson et al., we determine proper motions (PMs) in 14.60 arcmin X 16.53 arcmin area of the kinematically "thick-disk" globular cluster M12. The cluster's proximity and sparse nature makes it a…

星系天体物理 · 物理学 2018-10-17 Devesh P. Sariya , Ing-Guey Jiang , R. K. S. Yadav

We derive relative proper motions of stars in the fields of globular clusters M4, M12, M22, NGC 3201, NGC 6362 and NGC 6752 based on a uniform data set collected between 1997 and 2008. We assign a membership class for each star with a…

太阳与恒星天体物理 · 物理学 2013-01-15 K. Zloczewski , J. Kaluzny , M. Rozyczka , W. Krzeminski , B. Mazur , I. B. Thompson

We have developed a new procedure to identify moving groups, and have applied it to carry out a census of the nearby OB associations based on Hipparcos parallaxes and proper motions (see de Bruijne et al. and de Zeeuw et al. elsewhere in…

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

The comparison of the proper motions constructed from positions spanning a short (Hipparcos) or long time (Tycho-2) makes it possible to uncover binaries with periods of the order of or somewhat larger than the short time span, since the…

天体物理学 · 物理学 2009-11-11 A. Frankowski , S. Jancart , A. Jorissen

The Tycho-Gaia Astrometric Solution (TGAS) subset of the first Gaia catalogue contains an unprecedented sample of proper motions and parallaxes for two million stars brighter than G~12 mag. We take advantage of the full astrometric solution…

A comprehensive census of the stellar content of the nearby OB associations is presented, based on Hipparcos positions, proper motions, and parallaxes. Moving groups are identified by combining de Bruijne's refurbished convergent point…

天体物理学 · 物理学 2009-10-30 P. T. de Zeeuw , R. Hoogerwerf , J. H. J. de Bruijne , A. G. A. Brown , A. Blaauw

The main objective of this work is to determine the cluster members of 1876 open clusters, using positions and proper motions of the astrometric catalogue UCAC4. For this purpose we apply three different methods, all them based on a…

太阳与恒星天体物理 · 物理学 2017-07-26 L. Sampedro , W. S. Dias , E. J. Alfaro , H. Monteiro , A. Molino

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

Interstellar polarimetric data of the six open clusters Hogg 15, NGC 6611, NGC 5606, NGC 6231, NGC 5749 and NGC 6250 have been used to estimate the membership probability for the stars within them. For proper-motion member stars, the…

星系天体物理 · 物理学 2015-06-12 Biman J. Medhi , Motohide Tamura

A summary is given of an analysis of the Hipparcos trigonometrical parallaxes and proper motions of classical Cepheids. It is possible for the first time to derive zero-points for the period-luminosity and period-luminosity-colour relations…

天体物理学 · 物理学 2007-05-23 M. W. Feast , P. A. Whitelock