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Related papers: Local stellar kinematics from Hipparcos data

200 papers

We use the method of statistical parallax to constrain the distance-scale zero points and analyze the kinematics of extensive samples of Galactic classical Cepheids, RR Lyrae type variables, and blue horizontal branch stars, which serve as…

Astrophysics of Galaxies · Physics 2010-01-12 A. K. Dambis

The space velocities from the catalog of Nordstrom et al. (2004) are used to trace variations of a number of kinematic parameters of single F and G dwarfs as a function of their age. The vertex deviation of disk stars increases from 7+- 1…

Astrophysics · Physics 2009-06-23 Vadim V. Bobylev , Anisa T. Bajkova

We reanalyse the measurements of parallax, proper motion, and line-of-sight velocity for 18 masers in high mass star-forming regions presented by Reid et al. (2009). We use a likelihood analysis to investigate the distance of the Sun from…

Astrophysics of Galaxies · Physics 2015-05-13 Paul J. McMillan , James J. Binney

[abridged] A "missing data" algorithm is developed to model (ie, reconstruct) the three-dimensional velocity distribution function of a sample of stars using data (velocity measurements) every one of which has one dimension unmeasured (the…

Astrophysics · Physics 2009-11-11 David W. Hogg , Michael R. Blanton , Sam T. Roweis , Kathryn V. Johnston

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…

Astrophysics · Physics 2015-06-24 Michael Feast , Patricia Whitelock

In previous works of this series, we have shown that late B- and early A-type stars have genuine bimodal distributions of rotational velocities and that late A-type stars lack slow rotators. The distributions of the surface angular velocity…

Solar and Stellar Astrophysics · Physics 2015-06-03 J. Zorec , F. Royer

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…

Astrophysics of Galaxies · Physics 2009-07-24 Jo Bovy , David W. Hogg , Sam T. Roweis

We have used integral field spectroscopy of a sample of six nearby (z~0.01-0.04) high star-formation rate (SFR~10-40 solar masses per year) galaxies to investigate the relationship between local velocity dispersion and star formation rate…

Astrophysics of Galaxies · Physics 2016-03-23 Mathew Varidel , Michael Pracy , Scott Croom , Matt Owers , Elaine Sadler

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;…

Astrophysics · Physics 2009-10-31 B. Fuchs , H. Jahreiss , R. Wielen

To estimate the peculiar velocity of the Sun with respect to the Local Standard of Rest (LSR), we used young objects in the Solar neighborhood with distance measurement errors within 10%-15%. These objects were the nearest Hipparcos stars…

Astrophysics of Galaxies · Physics 2015-06-19 Vadim Bobylev , Anisa Bajkova

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…

Astrophysics · Physics 2007-05-23 Carlos Abad , Katherine Vieira

We present a comparison of the observed, spatially integrated stellar and ionized gas velocity dispersions of $\sim1000$ massive ($\log M_{\star}/M_{\odot}\gtrsim\,10.3$) galaxies in the Large Early Galaxy Astrophysics Census (LEGA-C)…

We test the long-term kinematical stability of a Galactic stellar halo model, due to Kafle, et al. (2012), who study the kinematics of approximately 5000 blue horizontal branch (BHB) stars in the Sloan Digital Sky Survey (SDSS). The…

Astrophysics of Galaxies · Physics 2015-07-03 Sarah A. Bird , Chris Flynn

We have studied the kinematic properties of young pre-main-sequence stars. We have selected these stars based on data from the Gaia DR2 catalogue by invoking a number of photometric infrared surveys. Using 4564 stars with parallax errors…

Astrophysics of Galaxies · Physics 2020-11-03 V. V. Bobylev , A. T. Bajkova

In the solar-neighbourhood, older stars have larger random velocities than younger ones. It is argued that the increase in velocity dispersion with time is predominantly a gradual process rather than one induced by discrete events such as…

Astrophysics · Physics 2007-05-23 James Binney

We use stellar proper motions from the TGAS catalog to study the kinematics of OB-associations. The TGAS proper motions of OB-associations generally agree well with the Hipparcos proper motions. The parameters of the Galactic rotation curve…

Astrophysics of Galaxies · Physics 2017-10-11 A. M. Mel'nik , A. K. Dambis

We report a tight linear relation between the HI circular velocity measured at 6 $R_{\rm e}$ and the stellar velocity dispersion measured within 1 $R_{\rm e}$ for a sample of 16 early-type galaxies with stellar mass between $10^{10}$ and…

Astrophysics of Galaxies · Physics 2016-05-25 Paolo Serra , Tom Oosterloo , Michele Cappellari , Milan den Heijer , Gyula I. G. Józsa

To estimate the peculiar velocity of the Sun with respect to the Local Standard of Rest (LSR), we used young objects in the Solar neighborhood with distance measurement errors within 10%-15%. These objects were the nearest Hipparcos stars…

Astrophysics of Galaxies · Physics 2018-03-14 V. V. Bobylev , A. T. Bajkova

The kinematic parameters identified from high-velocity stars situated within 100 kpc are examined and analyzed. We included three high velocity programs comprising 591, 87, and 519 stars as a function of distances ranging from 0.10 to…

Solar and Stellar Astrophysics · Physics 2025-01-23 W. H. Elsanhoury

We analyze the 3D kinematics of a sample of $\sim 4400$ red clump stars ranging between 5 and 10 kpc from the Galactic center and up to 3 kpc from the Galactic plane. This sample is representative for the metal-rich ([Fe/H] = -0.6 to 0.5)…

Astrophysics of Galaxies · Physics 2015-05-20 D. I. Casetti-Dinescu , T. M. Girard , V. I. Korchagin , W. F van Altena