Hostname: page-component-745bb68f8f-g4j75 Total loading time: 0 Render date: 2025-01-27T12:20:44.919Z Has data issue: false hasContentIssue false
  • English
  • Français

Research of the Kinematic of the Gould Belt

Published online by Cambridge University Press:  07 August 2017

Tongqi Xu  and
Qing Lin
Tongqi Xu
Affiliation:
Shanghai Observatory, Academia Sinica 200030 Shanghai, China PR
Qing Lin
Affiliation:
Shanghai Observatory, Academia Sinica 200030 Shanghai, China PR

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Using the proper motions, radial velocities and distances of bright O, B stars taken from the FK5/FK5 suppl. stars, the velocity field of the Gould belt stars has been analysed. The results have been compared with that of the FK4 stars given by Fricke and Tsioumis.

Type
Impact on Astrophysics
Information
Symposium - International Astronomical Union , Volume 156: Developments in Astrometry and their Impacts on Astrophysics , 1993 , pp. 237 - 241
Copyright
Copyright © Kluwer 

References

Fricke, W. and Tsioumis, A. (1975) Astron. Astrophys. 42, 449 Google Scholar
Fricke, W. (1977) Veröffentlichungen Astronomisches Rechen-Institut, No.28.Google Scholar
Hoffleit, E.D. and Warren, W. (1988) The Bright Star Catalogue, 5th Edition, Yale University Observatory.Google Scholar
van Altena, W.F., Lee, J.T., and Hoffleit, E.D. (1991) The General Catalogue of Trigonometric Stellar Parallaxes, Yale University Observatory.Google Scholar