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Issue Astron. Astrophys. Suppl. Ser.
Volume 126, Number 3, December_II 1997
Page(s) 555 - 561
DOI http://dx.doi.org/10.1051/aas:1997282

DOI: 10.1051/aas:1997282

A&A Supplement series, Vol. 126, December II 1997, 555-561

Received March 4; accepted April 1, 1997

ICCD speckle observations of binary stars: Measurements during 1994-1995 gif

E. Aristiditex2html_wrap559 - M. Carbillettex2html_wrap559 - J.-L. Prieurtex2html_wrap563 - B. Lopeztex2html_wrap565 - Y. Bressontex2html_wrap565 - L. Koechlintex2html_wrap563

Send offprint request: E. Aristidi

tex2html_wrap571  UMR 6525 Astrophysique, Université de Nice Sophia, Antipolis, Centre National de la Recherche Scientifique, Parc Valrose, F-06108 Nice Cedex 2, France
tex2html_wrap573  Observatoire Midi Pyrénées, 14 Av. Edouard Belin, F-31000 Toulouse, France
tex2html_wrap575  UMR 6528, Département Fresnel de l'Observatoire de la Côte d'Azur, BP. 4229, F-06304 Nice Cedex 4, France

Abstract:

We present speckle observations of nineteen double stars and the triple star 2Cam. Angular separations, absolute position angles and relative photometry result from these observations. The angular separation is derived from the power spectrum. The position angle and the relative photometry are determined by two recent techniques: the cross-correlation between the speckle images and their square, and the ratios of twofold probability density functions of the images.

keywords: methods: data analysis -- techniques: image processing -- techniques: interferometric -- binaries: close

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