Astron. Astrophys. 358, L63-L66 (2000)

Letter to the Editor

Kinematics versus X-ray luminosity segregation in the Hyades

V.V. Makarov

Copenhagen University Observatory, Juliane Maries Vej 30, 2100 Copenhagen O, Denmark (makarov@astro.ku.dk)
DASGAL, Observatoire de Paris-Meudon, bat 11, 5 place Janssen, 92195 Meudon Cedex, France

Received 23 March 2000 / Accepted 19 May 2000

Abstract

State of the art Tycho-2 proper motions of bona fide Hyades members are used in combination with the ROSAT X-ray survey of this open cluster in Stern et al. (1995) to study the internal velocity dispersion versus X-ray luminosity by the classical convergent point method. It is shown in this paper for the Hyades members with below 0.7 mag that stars brighter than erg s^-1 (0.1-1.8 keV) have much more coherent motions than those with smaller X-ray luminosities and those not detected by ROSAT at all. In fact, the proper motions of the X-ray luminous members are in agreement with a null internal dispersion of velocities for this subpopulation, whereas the intermediate bright X-ray stars exhibit a dispersion at 320 m s^-1. The non-emitters, despite their being more massive and optically brighter, have a velocity dispersion of about 440 m s^-1. Probably related to this fact, the strong X-ray emitters are more concentrated within the tidal radius (10 pc) of the cluster centre than the non-emitters. Nearly half of strong X-ray emitters with coherent motions are visual or orbiting pairs with typical separations 5 to 50 AU. This find implies that a group of intermediate mass (1.0 to 1.5 solar masses) stars in the Hyades is significantly younger than the rest and their system is not yet dynamically relaxed.

Key words: Galaxy: open clusters and associations: individual: Hyades stars: kinematics X-rays: stars

SIMBAD Objects

Contents

• Text
• Acknowledgements
• References

© European Southern Observatory (ESO) 2000

Online publication: June 20, 2000
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