Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-26T04:32:21.039Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometric Observations of Three Double Stars by the Occultation Method — Comparison with Interferometric Results and with Preliminary Results of HIPPARCOS

Published online by Cambridge University Press:  12 April 2016

M. Froeschlé  and
C. Meyer
M. Froeschlé
Affiliation:
OCA/CERGA, Avenue Copernic, F – 06130 Grasse, France
C. Meyer
Affiliation:
OCA/CERGA, Avenue Copernic, F – 06130 Grasse, France

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.

We first briefly recall the geometry of the occultation of a double star by the Moon’s edge. Then we give a short description of the principle of the formation of the diffraction pattern. We present the results for three double stars and compare them with those obtained by other methods.

Type
High Resolution At Visual Wavelengths
Information
International Astronomical Union Colloquium , Volume 135: Complementary Approaches to Double and Multiple Star Research , 1992 , pp. 546 - 548
Copyright
Copyright © Astronomical Society of the Pacific 1992

References

McAlister, H.A. & Hartkopf, W.I., 1988 Second Catalog of interferometric measurements of binary stars, CHARA Contribution No. 2.Google Scholar
Schmidtke, P.C., Africano, J.L., & Quigley, R., 1989, AJ, 97, 909 CrossRefGoogle Scholar