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相关论文: Improved Methods for Identifying Moving Groups

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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

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

A new method to identify coherent structures in velocity space --- moving groups --- in astrometric catalogues is presented: the Spaghetti method. It relies on positions, parallaxes, and proper motions and is ideally suited to search for…

天体物理学 · 物理学 2009-10-31 R. Hoogerwerf , L. A. Aguilar

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

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 describe a procedure to identify stars from nearby moving groups and associations out of catalogs of stars with large proper motions. We show that from the mean motion vector of a known or suspected moving group, one can identify…

天体物理学 · 物理学 2009-11-13 Sebastien Lepine , Michal Simon

Proper motion measurements of the cool and ultracool populations in the Upper Scorpius OB association are crucial to confirm membership and to identify possible run-away objects. We cross-match samples of photometrically selected and…

太阳与恒星天体物理 · 物理学 2015-05-13 Herve Bouy , Eduardo L. Martin

We present a new high-mass membership of the nearby Sco OB2 association based on HIPPARCOS positions, proper motions and parallaxes and radial velocities taken from the Kharchenko et al. (2007) catalogue. The Bayesian membership selection…

太阳与恒星天体物理 · 物理学 2015-05-28 A. C. Rizzuto , M. J. Ireland , J. G. Robertson

We present the first results of a comprehensive census of the stellar content of the nearby OB associations based on Hipparcos positions, proper motions and parallaxes for 12842 candidate member stars distributed over 21 fields on the sky.…

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

Context: Convergent point (CP) search methods are important tools for studying the kinematic properties of open clusters and young associations whose members share the same spatial motion. Aims: We present a new CP search strategy based on…

天体物理仪器与方法 · 物理学 2011-12-16 P. A. B. Galli , R. Teixeira , C. Ducourant , C. Bertout , P. Benevides-Soares

To improve the census of the Upper Sco association (~11 Myr, ~145 pc), we have identified candidate members using parallaxes, proper motions, and color-magnitude diagrams from several wide-field imaging surveys and have obtained optical and…

太阳与恒星天体物理 · 物理学 2018-08-08 K. L. Luhman , K. A. Herrmann , E. E. Mamajek , T. L. Esplin , M. J. Pecaut

This paper is dedicated to investigating the kinematic properties of the Lupus moving group of young stars with the primary objective of deriving individual parallaxes for each group member. We identify those stars in the Lupus star-forming…

星系天体物理 · 物理学 2013-10-01 P. A. B. Galli , C. Bertout , R. Teixeira , C. Ducourant

Two motions in the galactic plane have been detected and characterized, based on the determination of a common systematic component in Hipparcos catalogue proper motions. The procedure is based only on positions, proper motions and…

天体物理学 · 物理学 2007-05-23 Carlos Abad , Katherine Vieira

We present a kinematic study of the Scorpius-Centaurus (Sco-Cen) OB association (Sco OB2) using Gaia DR1 parallaxes and proper motions. Our goal is to test the classical theory that OB associations are the expanded remnants of dense and…

太阳与恒星天体物理 · 物理学 2018-02-14 Nicholas J. Wright , Eric E. Mamajek

Scorpius-Centaurus is the nearest OB association and its hundreds of members were divided into sub-groups, including Lower Centaurus Crux. Here we study the dynamics of the Lower Centaurus Crux area stellar content. We report the revelation…

太阳与恒星天体物理 · 物理学 2018-11-28 Bertrand Goldman , Siegfried Roeser , Elena Schilbach , Attila C. Moór , Thomas Henning

Mean proper motions and parallaxes of 205 open clusters were determined from their member stars found in the Hipparcos Catalogue. 360 clusters were searched for possible members, excluding nearby clusters with distances D < 200 pc. Members…

天体物理学 · 物理学 2009-10-31 H. Baumgardt , C. Dettbarn , R. Wielen

We present results from a large spectroscopic survey of the nearest young association to the Sun, Upper Scorpius, conducted using 2dF/HERMES on the Anglo-Australian Telescope. We use spectroscopic youth criteria such as Li-equivalent widths…

We present continued results from a wide-field, ~150 deg^2, optical photometric and spectroscopic survey of the northern part of the ~5 Myr-old Upper Scorpius OB Association. Photometry and spectral types were used to derive effective…

天体物理学 · 物理学 2009-11-13 Catherine L. Slesnick , Lynne A. Hillenbrand , John M. Carpenter

A method for online identification of group of moving objects in the video is proposed in this paper. This method at each frame identifies group of tracked objects with similar local instantaneous motion pattern using spectral clustering on…

计算机视觉与模式识别 · 计算机科学 2019-09-04 Vahid Bastani , Damian Campo , Lucio Marcenaro , Carlo S. Regazzoni

Young nearby moving groups are important and useful in many fields of astronomy such as studying exoplanets, low-mass stars, and the stellar evolution of the early planetary systems over tens of millions of years, which has led to intensive…

太阳与恒星天体物理 · 物理学 2018-02-21 Jinhee Lee , Inseok Song
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