Kinematics of W Ursae Majoris type binaries and evidence of the two types of formation
Open Access
- 1 February 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 357 (2), 497-517
- https://doi.org/10.1111/j.1365-2966.2005.08609.x
Abstract
No abstract availableKeywords
This publication has 70 references indexed in Scilit:
- Reality Tests of Superclusters in the Young Disk PopulationThe Astronomical Journal, 1995
- Kinematics and age of RS Canum Venaticorum and by Draconis starsThe Astrophysical Journal Supplement Series, 1992
- Large and kinematically unbiased samples of G- and K-type stars. IV - Evolved stars of the old disk populationPublications of the Astronomical Society of the Pacific, 1989
- The spectroscopic orbits of BV and BW DraconisPublications of the Astronomical Society of the Pacific, 1986
- A spectrographic orbit for the eclipsing binary V757 CentauriPublications of the Astronomical Society of the Pacific, 1982
- The FK Comae starsThe Astrophysical Journal, 1981
- The Rapidly Rotating Giants of the FK Comae-TypePublished by Springer Science and Business Media LLC ,1981
- The orbital elements of W Ursae Majoris systemsVistas in Astronomy, 1970
- Stellar groups. II. The Herculis, Indi and 61 Cygni Groups of High-Velocity StarsMonthly Notices of the Royal Astronomical Society, 1958
- Stellar Groups. I. The Hyades and Sirius GroupsMonthly Notices of the Royal Astronomical Society, 1958