Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-27T00:34:39.644Z Has data issue: false hasContentIssue false

Designation of Multiple-star Components

Published online by Cambridge University Press:  30 March 2016

Andrei Tokovinin*
Affiliation:
Association of Universities for Research in Astronomy, Cerro Tololo Interamerican Observatory

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.

Hierarchical multiple stars need designations for individual components, for super-components (several bodies that act as single dynamical center and are often measured jointly) and sub-systems. Hierarchical designations like those proposed for WMC can satisfy all needs, but designations will have to be frozen and will not reflect true hierarchy in the future as new components are discovered. Hence, a clearing house (WMC on the web?) is needed to maintain unique and consistent designations. The hierarchy can be coded separately and flexibly by reference to parent super-components. As an example, these ideas are applied to a real quintuple star HR 1706.

Type
II. Special Scientific Sessions
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Barstow, M.A., Bond, H.E., Burleigh, M.R., Holberg, J.B., 2001 MNRAS, 322, 891 Google Scholar
Hartkopf, W.I., & Mason, B. D. Addressing confusion in double star nomenclature: The Washington Multiplicity Catalog , 2004, IAU Colloq. 191, THE ENVIRONMENTS AND EVOLUTION OF DOUBLE AND MULTIPLE STARS, Mérida, Yucatán, México, Allen, C. and Scarfe, C., editors, RevMexAA(SC), in pressGoogle Scholar
Mason, B.D., Wycoff, G.L., and Hartkopf, W.I., 2003, The Washington Double Star Catalog Google Scholar
Tokovinin, A.A. 1997a A&AS, 121, 71 Google Scholar
Tokovinin, A.A. 1997b A&AS, 124, 75 Google Scholar