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相关论文: A Precision test of Hipparcos systematics towards …

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We reconsider calibration of statistical distance scales for planetary nebulae, examining precision and systematic error for various distance methods used as well as the scales themselves. A different calibration strategy, one based on…

太阳与恒星天体物理 · 物理学 2015-06-22 Haywood Smith

Parallax data from the Hipparcos mission allow the direct distance to open clusters to be compared with the distance inferred from main sequence (MS) fitting. There are surprising differences between the two distance measurements, which…

天体物理学 · 物理学 2009-09-07 Marc H. Pinsonneault , John Stauffer , David R. Soderblom , Jeremy King , Robert B. Hanson

The Hyades cluster is an ideal target to study the dynamical evolution of a star cluster over the entire mass range due to its intermediate age and proximity to the Sun. We wanted to extend the Hyades mass function towards lower masses down…

Velocity dispersions have been employed as a method to measure masses of clusters. To complement this conventional method, we explore the possibility of constraining cluster masses from the stacked phase space distribution of galaxies at…

星系天体物理 · 物理学 2019-09-04 Akinari Hamabata , Masamune Oguri , Takahiro Nishimichi

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 new BVRI photometry for a sample of 54 local G and K stars with accurate Hipparcos parallaxes in the metallicity range -0.4 < [Fe/H] < +0.3. We use this sample to develop a completely model-independent main sequence (MS) fitting…

天体物理学 · 物理学 2011-05-23 Susan M. Percival , Maurizio Salaris , David Kilkenny

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

Since the release of the Hipparcos catalog in 1997, the distance to the Pleiades open cluster has been heavily debated. The distance obtained from Hipparcos and those by alternative methods differ by 10 to 15 %. As accurate stellar…

Because of its proximity and its youth, the Pleiades open cluster of stars has been extensively studied and serves as a cornerstone for our understanding of the physical properties of young stars. This role is called into question by the…

太阳与恒星天体物理 · 物理学 2015-06-22 Carl Melis , Mark J. Reid , Amy J. Mioduszewski , John R. Stauffer , Geoffrey C. Bower

Three binary systems in the Hyades open cluster (51 Tau, V818 Tau, and $\theta^2$ Tau}, with known metallicity and good Johnson photometric data are used to test the validity of three independent sets of stellar evolutionary tracks. A…

天体物理学 · 物理学 2007-05-23 E. Lastennet , D. Valls-Gabaud , T. Lejeune , E. Oblak

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

Using the Gaia colour-magnitude diagram, we assign masses to a catalogue of 979 confirmed members of the Hyades cluster and tails. By fitting the cumulative mass profile, stars within the tidal radius have a Plummer-like profile with…

星系天体物理 · 物理学 2022-03-30 N. Wyn Evans , Semyeong Oh

We present a three-dimensional reconstruction of the velocity distribution of nearby stars (<~ 100 pc) using a maximum likelihood density estimation technique applied to the two-dimensional tangential velocities of stars. The underlying…

星系天体物理 · 物理学 2009-07-24 Jo Bovy , David W. Hogg , Sam T. Roweis

The parallaxes determined by Lacy (1979) by means of eclipsing binaries method are compared with the Hipparcos parallaxes for 19 systems. The residual scatter of the distance moduli inferred from eclipsing binaries method - after allowing…

天体物理学 · 物理学 2007-05-23 Irena Semeniuk

We present a mathematical analysis of the statistical parallax method. The method yields physical insight into the maximum-likelihood determinations of the luminosity and velocity distribution and enables us to conduct a vigorous Monte…

天体物理学 · 物理学 2008-02-03 Piotr Popowski , Andrew Gould

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 review seven methods of measuring the absolute magnitude M_V of RR Lyrae stars in light of the Hipparcos mission and other recent developments. We focus on identifying possible systematic errors and rank the methods by relative immunity…

天体物理学 · 物理学 2016-01-27 Piotr Popowski , Andrew Gould

We present astrometric results from a Hubble Space Telescope (HST) campaign aimed at determining precise distances for cold Y-type brown dwarfs. Combining observations from a dedicated HST/WFC3 program with archival data, we derive…

太阳与恒星天体物理 · 物理学 2025-01-09 Clémence Fontanive , Luigi R. Bedin , Loïc Albert , Daniella C. Bardalez Gagliuffi

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

A study of cluster characteristics and internal kinematical structure of the middle-aged Pleiades open star cluster is presented. The individual star apexes and various cluster kinematical parameters including the velocity ellipsoid…

太阳与恒星天体物理 · 物理学 2018-03-21 W. H. Elsanhoury , E. S. Postnikova , N. V. Chupina , S. V. Vereshchagin , Devesh P. Sariya , R. K. S. Yadav , Ing-Guey Jiang