Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-25T16:49:46.075Z Has data issue: false hasContentIssue false
  • English
  • Français

Maintenance of ICRP: Complex Optical Objects

Published online by Cambridge University Press:  14 August 2015

Charles E. Worley
Charles E. Worley*
Affiliation:
U.S. Naval Observatory, Washington D.C., USA

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.

Heretofore, double and multiple stars have presented a tolerable but manageable problem in most astrometric programs. However, the drive to ever greater precision, with detections in the milli-to-micro arcsecond range of these complex objects, over a wide range of wavelengths, presents new and as yet unsolved problems in both the astrometry and photometry of such systems.

This discussion is aimed at a better delineation of the implications of the problem.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 1: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part A), 1997 , 1998 , pp. 325
Copyright
Copyright © Kluwer 1998