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Double Star Speckle Interferometry with the 3.5-m Telescope at Calar Alto (Almería, Spain)

Published online by Cambridge University Press:  09 August 2007

J.A. Docobo
Affiliation:
Astronomical Observatory R. M. Aller, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Spain email: oadoco@usc.es
V.S. Tamazian
Affiliation:
Astronomical Observatory R. M. Aller, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Spain email: oadoco@usc.es
M. Andrade
Affiliation:
Astronomical Observatory R. M. Aller, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Spain email: oadoco@usc.es
J.F. Ling
Affiliation:
Astronomical Observatory R. M. Aller, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Spain email: oadoco@usc.es
Y.Y. Balega
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkesia 369167, Russia
J.F. Lahulla
Affiliation:
Observatorio Astronómico Nacional, Calle Alfonso XII 3, 28014 Madrid, Spain
A. Maximov
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkesia 369167, Russia
J.R. González–Romay
Affiliation:
Astronomical Observatory R. M. Aller, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Spain email: oadoco@usc.es
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Abstract

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The first results of speckle interferometry carried out with the 3.5-m telescope of the C.A.H.A. (Almería, Spain) during a run in July, 2005 are presented. Forty nine stars with separations between 0″058 and 2″1 were observed under good seeing conditions. On the basis of these observations three improved orbits are presented. The Time Allocation Committee's report with a high scientific qualification to our proposal is included. It confirms the relevance of binary and multiple star research in modern astronomy and the great significance of large telescopes in this kind of studies as well.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

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