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Binary Star Observations in Selected Instants of Good Seeing

Published online by Cambridge University Press:  05 March 2013

John Davis  and
Julian R. North
John Davis*
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Julian R. North
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
*
davis@physics.usyd.edu.au
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Abstract

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Video recordings of images of binary stars at the focus of a 0.36m telescope have been used to select images recorded in instants of good seeing. The selected images have been analysed to give separations and position angles for the binary systems which are in good agreement with values predicted from previous observations. In these exploratory observations it has been shown that separations of 0.9 arcseconds can be measured with an accuracy of ~2% and position angles to ~1–2 degrees when the average seeing was ~1.3 arcseconds. These observations demonstrated that the diffraction limit of the telescope could be reached when the seeing was a factor of 2–3 greater than it. A binary with three magnitudes difference in the brightness of its components has been measured with comparable accuracy although difficulties are anticipated for binaries with components closer than ~2 arcseconds with this magnitude difference. The limiting magnitude is determined by the need to limit exposure times of individual frames to be comparable with or less than the atmospheric coherence time.

Keywords

atmospheric effectsstars: binariestechniques: image processing
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 18 , Issue 3 , 2001 , pp. 281 - 286
Copyright
Copyright © Astronomical Society of Australia 2001

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